Merge branch 'master' of bitbucket.org:glavaux/cosmotool

This commit is contained in:
Guilhem Lavaux 2013-03-07 09:39:59 -06:00
commit 766c86247a
85 changed files with 4930 additions and 765 deletions

View File

@ -55,6 +55,7 @@ include(FindHDF5)
include(FindPkgConfig) include(FindPkgConfig)
pkg_check_modules(FFTW3 fftw3>=3.3) pkg_check_modules(FFTW3 fftw3>=3.3)
pkg_check_modules(FFTW3F fftw3f>=3.3)
pkg_check_modules(EIGEN3 eigen3) pkg_check_modules(EIGEN3 eigen3)
include(FindPackageHandleStandardArgs) include(FindPackageHandleStandardArgs)

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@ -0,0 +1,161 @@
#+
# This is CosmoTool (./build_tools/gather_sources.py) -- Copyright (C) Guilhem Lavaux (2007-2013)
#
# guilhem.lavaux@gmail.com
#
# This software is a computer program whose purpose is to provide a toolbox for cosmological
# data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
#
# This software is governed by the CeCILL license under French law and
# abiding by the rules of distribution of free software. You can use,
# modify and/ or redistribute the software under the terms of the CeCILL
# license as circulated by CEA, CNRS and INRIA at the following URL
# "http://www.cecill.info".
#
# As a counterpart to the access to the source code and rights to copy,
# modify and redistribute granted by the license, users are provided only
# with a limited warranty and the software's author, the holder of the
# economic rights, and the successive licensors have only limited
# liability.
#
# In this respect, the user's attention is drawn to the risks associated
# with loading, using, modifying and/or developing or reproducing the
# software by the user in light of its specific status of free software,
# that may mean that it is complicated to manipulate, and that also
# therefore means that it is reserved for developers and experienced
# professionals having in-depth computer knowledge. Users are therefore
# encouraged to load and test the software's suitability as regards their
# requirements in conditions enabling the security of their systems and/or
# data to be ensured and, more generally, to use and operate it in the
# same conditions as regards security.
#
# The fact that you are presently reading this means that you have had
# knowledge of the CeCILL license and that you accept its terms.
#+
import shutil
import tempfile
import re
from git import Repo,Tree,Blob
def apply_license(license, relimit, filename):
header = re.sub(r'@FILENAME@', filename, license)
f = file(filename)
lines = f.read()
f.close()
lines = re.sub(relimit, '', lines)
lines = header + lines
with tempfile.NamedTemporaryFile(delete=False) as tmp_sources:
tmp_sources.write(lines)
shutil.move(tmp_sources.name, filename)
def apply_python_license(filename):
license="""#+
# This is CosmoTool (@FILENAME@) -- Copyright (C) Guilhem Lavaux (2007-2013)
#
# guilhem.lavaux@gmail.com
#
# This software is a computer program whose purpose is to provide a toolbox for cosmological
# data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
#
# This software is governed by the CeCILL license under French law and
# abiding by the rules of distribution of free software. You can use,
# modify and/ or redistribute the software under the terms of the CeCILL
# license as circulated by CEA, CNRS and INRIA at the following URL
# "http://www.cecill.info".
#
# As a counterpart to the access to the source code and rights to copy,
# modify and redistribute granted by the license, users are provided only
# with a limited warranty and the software's author, the holder of the
# economic rights, and the successive licensors have only limited
# liability.
#
# In this respect, the user's attention is drawn to the risks associated
# with loading, using, modifying and/or developing or reproducing the
# software by the user in light of its specific status of free software,
# that may mean that it is complicated to manipulate, and that also
# therefore means that it is reserved for developers and experienced
# professionals having in-depth computer knowledge. Users are therefore
# encouraged to load and test the software's suitability as regards their
# requirements in conditions enabling the security of their systems and/or
# data to be ensured and, more generally, to use and operate it in the
# same conditions as regards security.
#
# The fact that you are presently reading this means that you have had
# knowledge of the CeCILL license and that you accept its terms.
#+
"""
print("Shell/Python file: %s" % filename)
relimit=r'^#\+\n(#.*\n)*#\+\n'
apply_license(license, relimit, filename)
def apply_cpp_license(filename):
license="""/*+
This is CosmoTool (@FILENAME@) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
"""
relimit = r'^(?s)/\*\+.*\+\*/'
print("C++ file: %s" % filename)
apply_license(license, relimit, filename)
def analyze_tree(prefix, t):
for ename,entry in t.items():
if ename == 'external' or ename == 'zobov':
continue
if type(entry) == Tree:
analyze_tree(prefix + "/" + ename, entry)
elif type(entry) == Blob:
if ename == './src/hdf5_flash.h' or ename == './src/h5_readFlash.cpp' or ename == './src/h5_readFlash.hpp':
continue
if re.match(".*\.(sh|py|pyx)$",ename) != None:
fname=prefix+"/"+ename
apply_python_license(fname)
if re.match('.*\.(cpp|hpp|h)$', ename) != None:
fname=prefix+"/"+ename
apply_cpp_license(fname)
if __name__=="__main__":
repo = Repo(".")
assert repo.bare == False
t = repo.tree()
analyze_tree(".", t)

View File

@ -20,6 +20,9 @@ target_link_libraries(testkd ${tolink})
add_executable(testkd2 testkd2.cpp) add_executable(testkd2 testkd2.cpp)
target_link_libraries(testkd2 ${tolink}) target_link_libraries(testkd2 ${tolink})
add_executable(testkd3 testkd3.cpp)
target_link_libraries(testkd3 ${tolink})
add_executable(testDelaunay testDelaunay.cpp) add_executable(testDelaunay testDelaunay.cpp)
target_link_libraries(testDelaunay ${tolink}) target_link_libraries(testDelaunay ${tolink})
@ -44,10 +47,10 @@ target_link_libraries(testAlgo ${tolink})
add_executable(testBSP testBSP.cpp) add_executable(testBSP testBSP.cpp)
target_link_libraries(testBSP ${tolink}) target_link_libraries(testBSP ${tolink})
if (FFTW3_FOUND AND EIGEN3_FOUND) if (FFTW3_FOUND AND FFTW3F_FOUND AND EIGEN3_FOUND)
add_executable(test_fft_calls test_fft_calls.cpp) add_executable(test_fft_calls test_fft_calls.cpp)
target_link_libraries(test_fft_calls ${tolink} ${FFTW3_LIBRARIES}) target_link_libraries(test_fft_calls ${tolink} ${FFTW3_LIBRARIES} ${FFTW3F_LIBRARIES})
endif (FFTW3_FOUND AND EIGEN3_FOUND) endif (FFTW3_FOUND AND FFTW3F_FOUND AND EIGEN3_FOUND)
if (SHARP_LIBRARY AND SHARP_INCLUDE_PATH AND EIGEN3_FOUND) if (SHARP_LIBRARY AND SHARP_INCLUDE_PATH AND EIGEN3_FOUND)
include_directories(${SHARP_INCLUDE_PATH}) include_directories(${SHARP_INCLUDE_PATH})
@ -55,3 +58,7 @@ if (SHARP_LIBRARY AND SHARP_INCLUDE_PATH AND EIGEN3_FOUND)
target_link_libraries(test_healpix_calls ${tolink} ${SHARP_LIBRARIES}) target_link_libraries(test_healpix_calls ${tolink} ${SHARP_LIBRARIES})
set_target_properties(test_healpix_calls PROPERTIES COMPILE_FLAGS ${OpenMP_CXX_FLAGS} LINK_FLAGS ${OpenMP_CXX_FLAGS}) set_target_properties(test_healpix_calls PROPERTIES COMPILE_FLAGS ${OpenMP_CXX_FLAGS} LINK_FLAGS ${OpenMP_CXX_FLAGS})
endif (SHARP_LIBRARY AND SHARP_INCLUDE_PATH AND EIGEN3_FOUND) endif (SHARP_LIBRARY AND SHARP_INCLUDE_PATH AND EIGEN3_FOUND)
add_executable(test_cosmopower test_cosmopower.cpp)
target_link_libraries(test_cosmopower ${tolink})

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testAlgo.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <iostream> #include <iostream>
#include <stdio.h> #include <stdio.h>
#include "algo.hpp" #include "algo.hpp"

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testBQueue.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <iostream> #include <iostream>
#include "bqueue.hpp" #include "bqueue.hpp"

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testBSP.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#if 0 #if 0
#include "bsp_simple.hpp" #include "bsp_simple.hpp"

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testDelaunay.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <fstream> #include <fstream>
#include <iostream> #include <iostream>
#include "dinterpolate.hpp" #include "dinterpolate.hpp"

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@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testEskow.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <fstream> #include <fstream>
#include <cstring> #include <cstring>
#include <iostream> #include <iostream>

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@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testInterpolate.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <iostream> #include <iostream>
#include "interpolate3d.hpp" #include "interpolate3d.hpp"

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testNewton.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <iostream> #include <iostream>
#include <cmath> #include <cmath>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testPool.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include "pool.hpp" #include "pool.hpp"
using namespace CosmoTool; using namespace CosmoTool;

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testReadFlash.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <iostream> #include <iostream>
#include <assert.h> #include <assert.h>
#include <stdio.h> #include <stdio.h>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testSmooth.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <iostream> #include <iostream>
#include "sphSmooth.hpp" #include "sphSmooth.hpp"
#include "yorick.hpp" #include "yorick.hpp"

View File

@ -0,0 +1,63 @@
/*+
This is CosmoTool (./sample/test_cosmopower.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <cmath>
#include <iostream>
#include "cosmopower.hpp"
using namespace std;
using namespace CosmoTool;
int main()
{
CosmoPower cp;
CosmoPower::CosmoFunction f[] = { CosmoPower::POWER_EFSTATHIOU, CosmoPower::HU_WIGGLES, CosmoPower::HU_BARYON, CosmoPower::POWER_SUGIYAMA };
int num_F = sizeof(f)/sizeof(f[0]);
cp.setFunction(f[0]);
cp.normalize();
for (int ik = 0; ik < 100; ik++)
{
double k = pow(10.0, 4*ik/100.-3);
cout << k << " ";
for (int q = 0; q < num_F; q++)
{
cp.setFunction(f[q]);
cout << cp.power(k) << " ";
}
cout << endl;
}
return 0;
}

View File

@ -1,20 +1,93 @@
/*+
This is CosmoTool (./sample/test_fft_calls.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <boost/format.hpp>
#include "yorick.hpp"
#include <gsl/gsl_rng.h>
#include <iostream> #include <iostream>
#include <cmath>
#include "fourier/euclidian.hpp" #include "fourier/euclidian.hpp"
using namespace CosmoTool; using namespace CosmoTool;
using boost::format;
using boost::str;
using namespace std; using namespace std;
int main() double spectrum_generator(double k)
{ {
EuclidianFourierTransform_2d<double> dft(128,128,1.0,1.0); if (k==0)
double volume = 128*128; return 0;
return 1/(0.01+pow(k, 3.0));
}
template<typename T>
void test_2d(int Nx, int Ny)
{
EuclidianFourierTransform_2d<T> dft(Nx,Ny,1.0,1.0);
EuclidianSpectrum_1D<T> spectrum(spectrum_generator);
double volume = Nx*Ny;
gsl_rng *rng = gsl_rng_alloc(gsl_rng_default);
dft.realSpace().eigen().setRandom(); dft.realSpace().eigen().setRandom();
dft.fourierSpace().scale(std::complex<T>(0,0));
dft.analysis(); dft.analysis();
cout << format("Testing (%d,%d)") % Nx % Ny << endl;
cout << "Map dot-product = " << dft.realSpace().dot_product(dft.realSpace()) << endl; cout << "Map dot-product = " << dft.realSpace().dot_product(dft.realSpace()) << endl;
cout << "Fourier dot-product = " << dft.fourierSpace().dot_product(dft.fourierSpace()).real()*volume << endl; cout << "Fourier dot-product = " << dft.fourierSpace().dot_product(dft.fourierSpace()).real()*volume << endl;
dft.synthesis(); dft.synthesis();
cout << "Resynthesis dot-product = " << dft.realSpace().dot_product(dft.realSpace()) << endl; cout << "Resynthesis dot-product = " << dft.realSpace().dot_product(dft.realSpace()) << endl;
return 0;
dft.realSpace().scale(2.0);
dft.fourierSpace().scale(0.2);
spectrum.newRandomFourier(rng, dft.fourierSpace());
dft.synthesis();
uint32_t dims[2] = { Ny, Nx };
CosmoTool::saveArray(str(format("generated_map_%d_%d.nc") %Nx % Ny) , dft.realSpace().data(), dims, 2);
gsl_rng_free(rng);
}
int main(int argc, char **argv)
{
test_2d<double>(128,128);
test_2d<double>(131,128);
test_2d<double>(130,128);
test_2d<float>(128,128);
test_2d<float>(128,131);
test_2d<float>(128,130);
return 0;
} }

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/test_healpix_calls.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <iostream> #include <iostream>
#include "fourier/healpix.hpp" #include "fourier/healpix.hpp"
@ -6,15 +41,20 @@ using namespace std;
int main() int main()
{ {
HealpixFourierTransform<double> dft(128,3*128,3*128, 40); HealpixFourierTransform<double> dft(128,2*128,2*128, 40);
HealpixUtilityFunction<double> utils;
long Npix = dft.realSpace().size(); long Npix = dft.realSpace().size();
dft.realSpace().eigen().setRandom(); dft.realSpace().eigen().setRandom();
dft.analysis(); dft.analysis();
cout << "Map dot-product = " << dft.realSpace().dot_product(dft.realSpace()) << endl; cout << "Map dot-product = " << dft.realSpace().dot_product(dft.realSpace()) << endl;
cout << "Fourier dot-product = " << dft.fourierSpace().dot_product(dft.fourierSpace()).real()*Npix/(4*M_PI) << endl; cout << "Fourier dot-product = " << dft.fourierSpace().dot_product(dft.fourierSpace()).real()*Npix/(4*M_PI) << endl;
cout << "Spectrum analysis" << endl;
HealpixUtilityFunction<double>::Spectrum_ptr s = utils.estimateSpectrumFromMap(dft.fourierSpace());
dft.synthesis(); dft.synthesis();
cout << "Resynthesis dot-product = " << dft.realSpace().dot_product(dft.realSpace()) << endl; cout << "Resynthesis dot-product = " << dft.realSpace().dot_product(dft.realSpace()) << endl;
return 0; return 0;
} }

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testkd.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#define __KD_TREE_SAVE_ON_DISK #define __KD_TREE_SAVE_ON_DISK
#include <ctime> #include <ctime>
#include <cassert> #include <cassert>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./sample/testkd2.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <ctime> #include <ctime>
#include <cassert> #include <cassert>
#include <cstdlib> #include <cstdlib>

187
sample/testkd3.cpp Normal file
View File

@ -0,0 +1,187 @@
/*+
This is CosmoTool (./sample/testkd3.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <ctime>
#include <cassert>
#include <cstdlib>
#include <iostream>
#include <fstream>
#define __KD_TREE_NUMNODES
#include "mykdtree.hpp"
#include "kdtree_splitters.hpp"
#include <limits>
#define NTRY 30
#define NGB 24
#define ND 3
using namespace std;
using namespace CosmoTool;
typedef KDTree<ND,char,ComputePrecision,KD_homogeneous_cell_splitter<ND, char> > MyTree;
//typedef KDTree<ND,char,ComputePrecision > MyTree;
typedef KDCell<ND,char> MyCell;
static double periodic(double a)
{
while (a < -0.5)
a+=1;
while (a > 0.5)
a -= 1;
return a;
}
MyCell *findNearest(MyTree::coords& xc, MyCell *cells, uint32_t Ncells)
{
MyCell *near2 = 0;
double R2 = INFINITY;
for (int i = 0; i < Ncells; i++)
{
double d2 = 0;
for (int j = 0; j < ND; j++)
{
double delta = periodic(xc[j]-cells[i].coord[j]);
d2 += delta*delta;
}
if (d2 < R2)
{
near2 = &cells[i];
R2 = d2;
}
}
return near2;
}
int main()
{
uint32_t Ncells = 3000000;
MyCell *cells = new MyCell[Ncells];
for (int i = 0; i < Ncells; i++)
{
cells[i].active = true;
for (int l = 0; l < ND; l++)
cells[i].coord[l] = drand48();
}
// Check timing
clock_t startTimer = clock();
MyTree tree(cells, Ncells);
clock_t endTimer = clock();
tree.setPeriodic(true, 1.0);
clock_t delta = endTimer-startTimer;
double myTime = delta*1.0/CLOCKS_PER_SEC * 1.0;
cout << "KDTree build = " << myTime << " s" << endl;
MyTree::coords *xc = new MyTree::coords[NTRY];
cout << "Generating seeds..." << endl;
for (int k = 0; k < NTRY; k++)
{
for (int l = 0; l < ND; l++)
xc[k][l] = drand48();
}
// Check consistency
cout << "Check consistency..." << endl;
MyCell **ngb = new MyCell *[NGB];
double *distances = new double[NGB];
ofstream fngb("nearest.txt");
for (int k = 0; k < NTRY; k++) {
cout << "Seed = " << xc[k][0] << " " << xc[k][1] << " " << xc[k][2] << endl;
tree.getNearestNeighbours(xc[k], NGB, ngb, distances);
int last = -1;
for (uint32_t i = 0; i < NGB; i++)
{
if (ngb[i] == 0)
continue;
last = i;
double d2 = 0;
for (int l = 0; l < 3; l++)
d2 += ({double delta = periodic(xc[k][l] - ngb[i]->coord[l]); delta*delta;});
fngb << ngb[i]->coord[0] << " " << ngb[i]->coord[1] << " " << ngb[i]->coord[2] << " " << sqrt(d2) << " " << sqrt(distances[i]) << endl;
}
fngb << endl << endl;
double farther_dist = distances[last];
for (uint32_t i = 0; i < Ncells; i++)
{
bool found = false;
// If the points is not in the list, it means it is farther than the farthest point
for (int j =0; j < NGB; j++)
{
if (&cells[i] == ngb[j]) {
found = true;
break;
}
}
double dist_to_seed = 0;
for (int l = 0; l < 3; l++)
{
double delta = periodic(xc[k][l]-cells[i].coord[l]);
dist_to_seed += delta*delta;
}
double delta_epsilon = fabs(farther_dist/dist_to_seed-1);
if (!found)
{
if (dist_to_seed <= farther_dist &&
delta_epsilon > 1000*sqrt(numeric_limits<double>::epsilon()))
{
cout << "SHOULD BE IN (d=" << dist_to_seed << "): Failed iteration " << k << " particle " << i << " (farthest=" << sqrt(farther_dist) << ")" << endl;
cout << "delta_epsilon = " << delta_epsilon << endl;
abort();
}
}
else
{
if (dist_to_seed > farther_dist &&
delta_epsilon > 1000*sqrt(numeric_limits<double>::epsilon()))
{
cout << "SHOULD BE OUT (d=" << sqrt(dist_to_seed) << "): Failed iteration " << k << " particle " << i << " (farthest=" << sqrt(farther_dist) << ")" << endl;
cout << "delta_epsilon = " << delta_epsilon << " epsilon = " << 100*sqrt(numeric_limits<double>::epsilon()) << endl;
abort();
}
}
}
}
return 0;
}

View File

@ -8,6 +8,7 @@ SET(CosmoTool_SRCS
powerSpectrum.cpp powerSpectrum.cpp
miniargs.cpp miniargs.cpp
growthFactor.cpp growthFactor.cpp
cosmopower.cpp
) )
IF(FOUND_NETCDF3) IF(FOUND_NETCDF3)

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/algo.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_ALGO_HPP #ifndef __COSMOTOOL_ALGO_HPP
#define __COSMOTOOL_ALGO_HPP #define __COSMOTOOL_ALGO_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/bqueue.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMO_QUEUE_HPP #ifndef __COSMO_QUEUE_HPP
#define __COSMO_QUEUE_HPP #define __COSMO_QUEUE_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/bsp_simple.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_SIMPLE_BSP_HPP #ifndef __COSMOTOOL_SIMPLE_BSP_HPP
#define __COSMOTOOL_SIMPLE_BSP_HPP #define __COSMOTOOL_SIMPLE_BSP_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/cic.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <assert.h> #include <assert.h>
#include <math.h> #include <math.h>
#include <inttypes.h> #include <inttypes.h>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/cic.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __CICFILTER_HPP #ifndef __CICFILTER_HPP
#define __CICFILTER_HPP #define __CICFILTER_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/config.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_CONFIG_HPP #ifndef __COSMOTOOL_CONFIG_HPP
#define __COSMOTOOL_CONFIG_HPP #define __COSMOTOOL_CONFIG_HPP

341
src/cosmopower.cpp Normal file
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@ -0,0 +1,341 @@
/*+
This is CosmoTool (./src/cosmopower.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <cassert>
#include <vector>
#include <algorithm>
#include <iostream>
#include <cmath>
#include <fstream>
#include <gsl/gsl_integration.h>
#include "cosmopower.hpp"
using namespace std;
using namespace CosmoTool;
#define USE_GSL
#define TOLERANCE 1e-6
#define NUM_ITERATION 8000
CosmoPower::CosmoPower()
{
eval = &CosmoPower::powerEfstathiou;
n = 1.0;
K0 = 1;
V_LG_CMB = 627;
CMB_VECTOR[0] = 56.759;
CMB_VECTOR[1] = -540.02;
CMB_VECTOR[2] = 313.50;
h = 0.719;
SIGMA8 = 0.77;
OMEGA_B = 0.043969;
OMEGA_C = 0.21259;
Theta_27 = 2.728/2.7;
updateCosmology();
}
/*
* This is \hat{tophat}
*/
static double tophatFilter(double u)
{
if (u != 0)
return 3 / (u*u*u) * (sin(u) - u * cos(u));
else
return 1;
}
static double powC(double q, double alpha_c)
{
return 14.2 / alpha_c + 386 / (1 + 69.9 * pow(q, 1.08));
}
static double T_tilde_0(double q, double alpha_c, double beta_c)
{
double a = log(M_E + 1.8 * beta_c * q);
return a / ( a + powC(q, alpha_c) * q * q);
}
static double j_0(double x)
{
if (x == 0)
return 1.0;
return sin(x)/x;
}
static double powG(double y)
{
double a = sqrt(1 + y);
return y * (-6 * a + (2 + 3 * y) *log((a + 1)/(a - 1)));
}
double CosmoPower::powerEfstathiou(double k)
{
double a = 6.4/Gamma0;
double b = 3/Gamma0;
double c = 1.7/Gamma0;
double nu = 1.13;
double f = (a*k) + pow(b*k,1.5) + pow(c*k,2);
// EFSTATHIOU ET AL. (1992)
return normPower * pow(k,n) * pow(1+pow(f,nu),(-2/nu));
}
double CosmoPower::powerHuWiggles(double k)
{
// EISENSTEIN ET HU (1998)
// FULL POWER SPECTRUM WITH BARYONS AND WIGGLES
double k_silk = 1.6 * pow(OMEGA_B * h * h, 0.52) * pow(OmegaEff, 0.73) * (1 + pow(10.4 * OmegaEff, -0.95));
double z_eq = 2.50e4 * OmegaEff * pow(Theta_27, -4);
double s = 44.5 * log(9.83 / OmegaEff) / (sqrt(1 + 10 * pow(OMEGA_B * h * h, 0.75)));
double f = 1 / (1 + pow(k * s / 5.4, 4));
double k_eq = 7.46e-2 * OmegaEff * pow(Theta_27, -2);
double a1 = pow(46.9 * OmegaEff, 0.670) * (1 + pow(32.1 * OmegaEff, -0.532));
double a2 = pow(12.0 * OmegaEff, 0.424) * (1 + pow(45.0 * OmegaEff, -0.582));
double alpha_c = pow(a1, -OMEGA_B/ OMEGA_0) * pow(a2, -pow(OMEGA_B / OMEGA_0, 3));
double q = k / (13.41 * k_eq);
double b1_betac = 0.944 * 1/(1 + pow(458 * OmegaEff, -0.708));
double b2_betac = pow(0.395 * OmegaEff, -0.0266);
double beta_c = 1/ ( 1 + b1_betac * (pow(OMEGA_C / OMEGA_0, b2_betac) - 1) );
double T_c = f * T_tilde_0(q, 1, beta_c) + (1 - f) * T_tilde_0(q, alpha_c, beta_c);
double b1_zd = 0.313 * pow(OmegaEff, -0.419) * (1 + 0.607 * pow(OmegaEff, 0.674));
double b2_zd = 0.238 * pow(OmegaEff, 0.223);
double z_d = 1291 * pow(OmegaEff, 0.251) / (1 + 0.659 * pow(OmegaEff, 0.828)) * (1 + b1_zd * pow(OmegaEff, b2_zd));
double R_d = 31.5 * OMEGA_B * h * h * pow(Theta_27, -4) * 1e3 / z_d;
double alpha_b = 2.07 * k_eq * s * pow(1 + R_d, -0.75) * powG((1 + z_eq)/(1 + z_d));
double beta_b = 0.5 + OMEGA_B / OMEGA_0 + (3 - 2 * OMEGA_B / OMEGA_0) * sqrt(pow(17.2 * OmegaEff, 2) + 1);
double beta_node = 8.41 * pow(OmegaEff, 0.435);
double s_tilde = s * pow(1 + pow(beta_node / (k * s), 3), -1./3);
double T_b = (T_tilde_0(q, 1, 1) / (1 + pow(k * s / 5.2, 2)) + alpha_b / (1 + pow(beta_b / (k * s), 3)) * exp(-pow(k/k_silk, 1.4))) * j_0(k * s_tilde);
double T_k = OMEGA_B/OMEGA_0 * T_b + OMEGA_C/OMEGA_0 * T_c;
return normPower * pow(k,n) * T_k * T_k;
}
double CosmoPower::powerHuBaryons(double k)
{
double s = 44.5 * log(9.83 / OmegaEff) / (sqrt(1 + 10 * pow(OMEGA_B * h * h, 0.75)));
double alpha_Gamma = 1 - 0.328 * log(431 * OmegaEff) * OMEGA_B / OMEGA_0 + 0.38 * log(22.3 * OmegaEff) * pow(OMEGA_B / OMEGA_0, 2);
double GammaEff = OMEGA_0 * h * (alpha_Gamma + (1 - alpha_Gamma)/(1 + pow(0.43 * k * s, 4)));
double q = k/(h*GammaEff) * pow(Theta_27, 2);
double L_0 = log(2 * M_E + 1.8 * q);
double C_0 = 14.2 + 731 / (1 + 62.5 * q);
double T0 = L_0 / (L_0 + C_0 * q * q);
return normPower * pow(k,n) * T0 * T0;
}
double CosmoPower::powerOld(double k)
{
static const double l = 1/(Omega * h*h);
static const double alpha = 1.7 * l, beta = 9.0 * pow(l, 1.5), gamma = l*l;
return normPower * pow(k,n) * pow(1 + alpha * k + beta * pow(k,1.5) + gamma *k*k,-2);
}
double CosmoPower::powerSugiyama(double k)
{
double q = k * Theta_27*Theta_27 / (OmegaEff * exp(-OMEGA_B - sqrt(h/0.5)*OMEGA_B/OMEGA_0));
double L0 = log(2*M_E + 1.8 * q);
double C0 = 14.2 + 731 / (1 + 62.5 * q);
double T_k = L0 / (L0 + C0 * q*q);
return normPower * pow(k,n) * T_k * T_k;
}
double CosmoPower::powerBardeen(double k)
{
double q = k / (OmegaEff);
double poly = 1 + 3.89 * q + pow(16.1*q,2) + pow(5.46*q,3) + pow(6.71*q,4);
double T_k = log(1+2.34*q)/(2.34*q) * pow(poly,-0.25);
return normPower * pow(k,n) * T_k * T_k;
}
double CosmoPower::powerBDM(double k)
{
k /= h*h;
double alpha1 = 190;
double Gmu = 4.6;
double alpha2 = 11.5;
double alpha3 = 11;
double alpha4 = 12.55;
double alpha5 = 0.0004;
return normPower*k*alpha1*alpha1*Gmu*Gmu/(1+(alpha2*k)+pow(alpha3*k,2)+pow(alpha4*k,3))*pow(1+pow(alpha5/k,2), -2);
}
double CosmoPower::powerTest(double k)
{
return 1/(1+k*k);
}
/*
* This function computes the normalization of the power spectrum. It requests
* a sigma8 (density fluctuations within 8 Mpc/h)
*/
static double gslPowSpecNorm(double k, void *params)
{
CosmoPower *c = (CosmoPower *)params;
return c->integrandNormalize(k);
}
double CosmoPower::integrandNormalize(double x)
{
double k = (1-x)/x;
double f = tophatFilter(k*8.0/h);
return power(k)*k*k*f*f/(x*x);
}
void CosmoPower::normalize()
{
double normVal = 0;
double abserr;
gsl_integration_workspace *w = gsl_integration_workspace_alloc(NUM_ITERATION);
gsl_function f;
f.function = gslPowSpecNorm;
f.params = this;
normPower = 1;
ofstream ff("PP_k.txt");
for (int i = 0; i < 100; i++)
{
double k = pow(10.0, 4.0*i/100.-2);
ff << k << " " << power(k) << endl;
}
// gsl_integration_qagiu(&f, 0, 0, TOLERANCE, NUM_ITERATION, w, &normVal, &abserr);
gsl_integration_qag(&f, 0, 1, 0, TOLERANCE, NUM_ITERATION, GSL_INTEG_GAUSS61, w, &normVal, &abserr);
gsl_integration_workspace_free(w);
normVal /= (2*M_PI*M_PI);
normPower = SIGMA8*SIGMA8/normVal;
}
void CosmoPower::updateCosmology()
{
OMEGA_0 = OMEGA_B+OMEGA_C;
Omega = OMEGA_0;
beta = pow(OMEGA_0, 5./9);
OmegaEff = OMEGA_0 * h * h;
Gamma0 = OMEGA_0 * h * h;
omega_B = OMEGA_B * h * h;
omega_C = OMEGA_C * h * h;
}
void CosmoPower::updatePhysicalCosmology()
{
OMEGA_B = omega_B / (h*h);
OMEGA_C = omega_C / (h*h);
OMEGA_0 = Gamma0 / (h*h);
beta = pow(OMEGA_0, 5./9);
}
double CosmoPower::eval_theta_theta(double k)
{
// Jennings (2012) fit
double P_deltadelta = power(k);
static const double alpha0 = -12480.5, alpha1 = 1.824, alpha2 = 2165.87, alpha3=1.796;
if (k > 0.3)
return 0;
double r =(alpha0*sqrt(P_deltadelta) + alpha1*P_deltadelta*P_deltadelta)/(alpha2 + alpha3*P_deltadelta);
assert(P_deltadelta > 0);
if (r < 0)
return 0;
return r;
}
double CosmoPower::power(double k)
{
return (this->*eval)(k);
}
void CosmoPower::setFunction(CosmoFunction f)
{
switch (f)
{
case POWER_EFSTATHIOU:
eval = &CosmoPower::powerEfstathiou;
break;
case HU_WIGGLES:
eval = &CosmoPower::powerHuWiggles;
break;
case HU_BARYON:
eval = &CosmoPower::powerHuBaryons;
break;
case OLD_POWERSPECTRUM:
eval = &CosmoPower::powerOld;
break;
case POWER_BARDEEN:
eval = &CosmoPower::powerBardeen;
break;
case POWER_SUGIYAMA:
eval = &CosmoPower::powerSugiyama;
break;
case POWER_BDM:
eval = &CosmoPower::powerBDM;
break;
case POWER_TEST:
eval = &CosmoPower::powerTest;
break;
default:
abort();
}
}
void CosmoPower::setNormalization(double A_K)
{
normPower = A_K/power(0.002);
}

109
src/cosmopower.hpp Normal file
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@ -0,0 +1,109 @@
/*+
This is CosmoTool (./src/cosmopower.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef _COSMOPOWER_HPP
#define _COSMOPOWER_HPP
namespace CosmoTool {
class CosmoPower
{
public:
// PRIMARY VARIABLES
double n;
double K0;
double V_LG_CMB;
double CMB_VECTOR[3];
double h;
double SIGMA8;
double OMEGA_B;
double OMEGA_C;
double omega_B;
double omega_C;
double Theta_27;
// DERIVED VARIABLES
double OMEGA_0;
double Omega;
double beta;
double OmegaEff;
double Gamma0;
double normPower;
enum CosmoFunction
{
POWER_EFSTATHIOU,
HU_WIGGLES,
HU_BARYON,
OLD_POWERSPECTRUM,
POWER_BARDEEN,
POWER_SUGIYAMA,
POWER_BDM,
POWER_TEST
};
CosmoPower();
void setFunction(CosmoFunction f);
void updateCosmology();
void updatePhysicalCosmology();
void normalize();
void setNormalization(double A_K);
double eval_theta_theta(double k);
double power(double k);
double integrandNormalize(double k);
private:
double (CosmoPower::*eval)(double);
double powerEfstathiou(double k);
double powerHuWiggles(double k);
double powerHuBaryons(double k);
double powerOld(double k);
double powerBardeen(double k);
double powerSugiyama(double k);
double powerBDM(double k);
double powerTest(double k);
};
};
#endif

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/dinterpolate.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMO_DINTERPOLATE_HPP #ifndef __COSMO_DINTERPOLATE_HPP
#define __COSMO_DINTERPOLATE_HPP #define __COSMO_DINTERPOLATE_HPP
@ -29,6 +64,7 @@ namespace CosmoTool {
uint32_t numSimplex; uint32_t numSimplex;
uint32_t *simplex_list; uint32_t *simplex_list;
gsl_eigen_symmv_workspace *eigen_work; gsl_eigen_symmv_workspace *eigen_work;
bool *disable_simplex;
/** /**
* This construct the interpolator. The construction is time consuming so * This construct the interpolator. The construction is time consuming so
@ -53,6 +89,7 @@ namespace CosmoTool {
this->simplex_list = simplex_list; this->simplex_list = simplex_list;
this->numPoints = numPoints; this->numPoints = numPoints;
this->numSimplex = numSimplex; this->numSimplex = numSimplex;
this->disable_simplex = new bool[numSimplex];
buildPreweight(); buildPreweight();
buildQuickAccess(); buildQuickAccess();
@ -67,6 +104,7 @@ namespace CosmoTool {
delete quickAccess; delete quickAccess;
delete[] point_to_simplex_list_base; delete[] point_to_simplex_list_base;
delete[] all_preweight; delete[] all_preweight;
delete[] disable_simplex;
gsl_eigen_symmv_free(eigen_work); gsl_eigen_symmv_free(eigen_work);
} }

View File

@ -1,3 +1,6 @@
#include <fstream>
#include <iostream>
#include <iomanip>
#include <cstdlib> #include <cstdlib>
#include <cassert> #include <cassert>
#include <gsl/gsl_matrix.h> #include <gsl/gsl_matrix.h>
@ -21,7 +24,8 @@ namespace CosmoTool {
for (uint32_t i = 0; i < (N+1)*numSimplex; i++) for (uint32_t i = 0; i < (N+1)*numSimplex; i++)
{ {
assert(simplex_list[i] < numPoints); assert(simplex_list[i] < numPoints);
numSimplex_by_point[simplex_list[i]]++; if (!disable_simplex[i/(N+1)])
numSimplex_by_point[simplex_list[i]]++;
} }
// Compute the total number and the index for accessing lists. // Compute the total number and the index for accessing lists.
@ -37,7 +41,11 @@ namespace CosmoTool {
{ {
for (int j = 0; j <= N; j++) for (int j = 0; j <= N; j++)
{ {
uint32_t p = simplex_list[(N+1)*i+j]; uint32_t s = (N+1)*i+j;
if (disable_simplex[i])
continue;
uint32_t p = simplex_list[s];
assert(index_by_point[p] < point_to_simplex_size); assert(index_by_point[p] < point_to_simplex_size);
point_to_simplex_list_base[index_by_point[p]] = i; point_to_simplex_list_base[index_by_point[p]] = i;
++index_by_point[p]; ++index_by_point[p];
@ -48,7 +56,9 @@ namespace CosmoTool {
for (uint32_t i = 0; i < numPoints; i++) for (uint32_t i = 0; i < numPoints; i++)
{ {
// check assertion // check assertion
assert((i==0 && index_by_point[0]==numSimplex_by_point[0]) || ((index_by_point[i]-index_by_point[i-1]) == (numSimplex_by_point[i]+1))); assert((i==0 && index_by_point[0]==numSimplex_by_point[0])
||
((index_by_point[i]-index_by_point[i-1]) == (numSimplex_by_point[i]+1)));
assert(index_by_point[i] < point_to_simplex_size); assert(index_by_point[i] < point_to_simplex_size);
point_to_simplex_list_base[index_by_point[i]] = -1; point_to_simplex_list_base[index_by_point[i]] = -1;
} }
@ -80,6 +90,7 @@ namespace CosmoTool {
double preweight[N*N]; double preweight[N*N];
double preweight_inverse[N*N]; double preweight_inverse[N*N];
gsl_permutation *p = gsl_permutation_alloc(N); gsl_permutation *p = gsl_permutation_alloc(N);
uint32_t numDisabled = 0;
all_preweight = new PType[N*N*numSimplex]; all_preweight = new PType[N*N*numSimplex];
@ -105,13 +116,38 @@ namespace CosmoTool {
gsl_linalg_LU_decomp(&M.matrix, p, &signum); gsl_linalg_LU_decomp(&M.matrix, p, &signum);
double a = fabs(gsl_linalg_LU_det(&M.matrix, signum)); double a = fabs(gsl_linalg_LU_det(&M.matrix, signum));
if (a < 1e-10) if (a < 1e-10)
throw InvalidArgumentException("Invalid tesselation. One simplex is coplanar."); {
gsl_linalg_LU_invert(&M.matrix, p, &iM.matrix); #ifdef DEBUG
for (int j = 0; j < N; j++)
{
PType xref = positions[pref][j];
for (int k = 0; k < N; k++)
{
preweight[j*N + k] = positions[simplex_list[k+base+1]][j] - xref;
}
}
std::ofstream f("matrix.txt");
for (int j = 0; j < N*N; j++)
f << std::setprecision(12) << preweight[j] << std::endl;
throw InvalidArgumentException("Invalid tesselation. One simplex is coplanar.");
#else
gsl_matrix_set_zero(&iM.matrix);
disable_simplex[i] = true;
numDisabled++;
#endif
}
else {
gsl_linalg_LU_invert(&M.matrix, p, &iM.matrix);
disable_simplex[i] = false;
}
for (int j = 0; j < N*N; j++) for (int j = 0; j < N*N; j++)
all_preweight[N*N*i + j] = preweight_inverse[j]; all_preweight[N*N*i + j] = preweight_inverse[j];
} }
std::cout << "Number of disabled simplices: " << numDisabled << std::endl;
gsl_permutation_free(p); gsl_permutation_free(p);
} }
@ -166,6 +202,9 @@ namespace CosmoTool {
template<typename PType, typename IType, int N> template<typename PType, typename IType, int N>
bool DelaunayInterpolate<PType,IType,N>::checkPointInSimplex(const CoordType& pos, uint32_t simplex) bool DelaunayInterpolate<PType,IType,N>::checkPointInSimplex(const CoordType& pos, uint32_t simplex)
{ {
if (disable_simplex[simplex])
return false;
uint32_t *desc_simplex = &simplex_list[simplex*(N+1)]; uint32_t *desc_simplex = &simplex_list[simplex*(N+1)];
CoordType *p[N+1], v[N], hyper; CoordType *p[N+1], v[N], hyper;

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/eskow.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __ESKOW_CHOLESKY_HPP #ifndef __ESKOW_CHOLESKY_HPP
#define __ESKOW_CHOLESKY_HPP #define __ESKOW_CHOLESKY_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/field.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_FIELD #ifndef __COSMOTOOL_FIELD
#define __COSMOTOOL_FIELD #define __COSMOTOOL_FIELD

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@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/fixArray.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __FIX_ARRAY_HPP #ifndef __FIX_ARRAY_HPP
#define __FIX_ARRAY_HPP #define __FIX_ARRAY_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/fortran.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include "config.hpp" #include "config.hpp"
#include <iostream> #include <iostream>
#include <fstream> #include <fstream>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/fortran.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMO_FORTRAN_HPP #ifndef __COSMO_FORTRAN_HPP
#define __COSMO_FORTRAN_HPP #define __COSMO_FORTRAN_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/fourier/base_types.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __BASE_FOURIER_TYPES_HPP #ifndef __BASE_FOURIER_TYPES_HPP
#define __BASE_FOURIER_TYPES_HPP #define __BASE_FOURIER_TYPES_HPP
@ -24,14 +59,28 @@ namespace CosmoTool
typedef Eigen::Map<VecType, Eigen::Aligned> MapType; typedef Eigen::Map<VecType, Eigen::Aligned> MapType;
typedef Eigen::Map<VecType const, Eigen::Aligned> ConstMapType; typedef Eigen::Map<VecType const, Eigen::Aligned> ConstMapType;
typedef FourierMap<std::complex<T> > FourierMapType; typedef FourierMap<std::complex<T> > FourierMapType;
typedef boost::shared_ptr<FourierMapType> FourierMapPtr;
typedef boost::shared_ptr<SpectrumFunction<T> > SpectrumFunctionPtr;
virtual boost::shared_ptr<FourierMapType> virtual ~SpectrumFunction() {}
newRandomFourier(gsl_rng *rng, const FourierMapType& like_map) const = 0;
virtual void mul(FourierMap<std::complex<T> >& m) const = 0; virtual void
newRandomFourier(gsl_rng *rng, FourierMapType& out_map) const = 0;
virtual SpectrumFunctionPtr copy() const = 0;
virtual const T *data() const { return 0; }
virtual const int *dof() const { return 0; }
virtual long size() const { return -1; }
virtual void sqrt() = 0;
virtual void mul(FourierMapType& m) const = 0;
virtual void mul_sqrt(FourierMapType& m) const = 0;
virtual void mul_inv(FourierMapType& m) const = 0;
virtual void mul_inv_sqrt(FourierMapType& m) const = 0;
}; };
template<typename T> template<typename T>
class FourierMap class FourierMap
{ {
@ -60,6 +109,12 @@ namespace CosmoTool
return ConstMapType(data(), size()); return ConstMapType(data(), size());
} }
FourierMap<T>& operator=(const FourierMap<T>& m)
{
eigen() = m.eigen();
return *this;
}
void sqrt() void sqrt()
{ {
MapType m = eigen(); MapType m = eigen();
@ -76,7 +131,7 @@ namespace CosmoTool
{ {
assert(size() == map2->size()); assert(size() == map2->size());
MapType m(data(), size()); MapType m(data(), size());
MapType m2(map2->data(), map2->size()); ConstMapType m2(map2->data(), map2->size());
m *= m2; m *= m2;
} }
@ -130,6 +185,18 @@ namespace CosmoTool
virtual void synthesis_conjugate() = 0; virtual void synthesis_conjugate() = 0;
}; };
template<typename T>
class MapUtilityFunction
{
public:
typedef SpectrumFunction<T> Spectrum;
typedef boost::shared_ptr<Spectrum> Spectrum_ptr;
typedef FourierMap<std::complex<T> > FMap;
virtual Spectrum_ptr estimateSpectrumFromMap(const FMap& m) const = 0;
virtual Spectrum_ptr newSpectrumFromRaw(T *data, long size,
const Spectrum& like_spec) const = 0;
};
}; };

View File

@ -0,0 +1,267 @@
/*+
This is CosmoTool (./src/fourier/details/euclidian_maps.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __DETAILS_EUCLIDIAN_MAPS
#define __DETAILS_EUCLIDIAN_MAPS
namespace CosmoTool
{
template<typename T>
class EuclidianFourierMapBase: public FourierMap<T>
{
public:
typedef std::vector<int> DimArray;
private:
boost::shared_ptr<T> m_data;
DimArray m_dims;
long m_size;
public:
EuclidianFourierMapBase(boost::shared_ptr<T> indata, const DimArray& indims)
{
m_data = indata;
m_dims = indims;
m_size = 1;
for (int i = 0; i < m_dims.size(); i++)
m_size *= m_dims[i];
}
virtual ~EuclidianFourierMapBase()
{
}
const DimArray& getDims() const { return m_dims; }
virtual const T *data() const { return m_data.get(); }
virtual T *data() { return m_data.get(); }
virtual long size() const { return m_size; }
virtual FourierMap<T> *copy() const
{
FourierMap<T> *m = this->mimick();
m->eigen() = this->eigen();
return m;
}
};
template<typename T>
class EuclidianFourierMapReal: public EuclidianFourierMapBase<T>
{
public:
typedef typename EuclidianFourierMapBase<T>::DimArray DimArray;
EuclidianFourierMapReal(boost::shared_ptr<T> indata, const DimArray& indims)
: EuclidianFourierMapBase<T>(indata, indims)
{}
virtual FourierMap<T> *mimick() const
{
return new EuclidianFourierMapReal<T>(
boost::shared_ptr<T>((T *)fftw_malloc(sizeof(T)*this->size()),
std::ptr_fun(fftw_free)),
this->getDims());
}
virtual T dot_product(const FourierMap<T>& other) const
throw(std::bad_cast)
{
const EuclidianFourierMapReal<T>& m2 = dynamic_cast<const EuclidianFourierMapReal<T>&>(other);
if (this->size() != m2.size())
throw std::bad_cast();
return (this->eigen()*m2.eigen()).sum();
}
};
template<typename T>
class EuclidianFourierMapComplex: public EuclidianFourierMapBase<std::complex<T> >
{
protected:
typedef boost::shared_ptr<std::complex<T> > ptr_t;
std::vector<double> delta_k;
int m_dim0;
bool even0, alleven;
long plane_size;
public:
typedef typename EuclidianFourierMapBase<std::complex<T> >::DimArray DimArray;
EuclidianFourierMapComplex(ptr_t indata,
int dim0,
const DimArray& indims,
const std::vector<double>& dk)
: EuclidianFourierMapBase<std::complex<T> >(indata, indims), delta_k(dk), m_dim0(dim0), even0((dim0 % 2)==0)
{
assert(dk.size() == indims.size());
plane_size = 1;
alleven = true;
for (int q = 1; q < indims.size(); q++)
{
plane_size *= indims[q];
alleven = alleven && ((indims[q]%2)==0);
}
}
virtual FourierMap<std::complex<T> > *mimick() const
{
return
new EuclidianFourierMapComplex<T>(
ptr_t((std::complex<T> *)
fftw_malloc(sizeof(std::complex<T>)*this->size()),
std::ptr_fun(fftw_free)),
m_dim0,
this->getDims(),
this->delta_k);
}
const std::vector<double>& get_delta_k() const
{
return this->delta_k;
}
template<typename Array, typename Array2>
void get_Kvec(const Array& ik, Array2& kvec) const
{
const DimArray& dims = this->getDims();
assert(ik.size() == dims.size());
assert(kvec.size() == dims.size());
kvec[0] = ik[0] * delta_k[0];
for (int q = 1; q < ik.size(); q++)
{
int dk = ik[q];
if (dk > dims[q]/2)
dk = dk - dims[q];
kvec[q] = dk*delta_k[q];
}
}
template<typename Array2>
void get_Kvec(long p, Array2& kvec) const
{
const DimArray& dims = this->getDims();
DimArray d(delta_k.size());
get_IKvec(p, d);
get_Kvec(d, kvec);
}
void get_IKvec(long p, DimArray& ikvec) const
{
const DimArray& dims = this->getDims();
assert(dims.size()==ikvec.size());
for (int q = 0; q < ikvec.size(); q++)
{
ikvec[q] = p%dims[q];
p = (p-ikvec[q])/dims[q];
}
}
template<typename Array>
double get_K(const Array& ik) const
{
const DimArray& dims = this->getDims();
assert(ik.size() == dims.size());
double k2 = 0;
k2 += CosmoTool::square(ik[0]*delta_k[0]);
for (int q = 1; q < ik.size(); q++)
{
int dk = ik[q];
if (dk > dims[q]/2)
dk = dk - dims[q];
k2 += CosmoTool::square(delta_k[q]*dk);
}
return std::sqrt(k2);
}
double get_K(long p) const
{
const DimArray& dims = this->getDims();
DimArray d(delta_k.size());
for (int q = 0; q < d.size(); q++)
{
d[q] = p%dims[q];
p = (p-d[q])/dims[q];
}
return get_K(d);
}
bool allDimensionsEven() const { return alleven; }
bool firstDimensionEven() const { return even0; }
virtual std::complex<T> dot_product(const FourierMap<std::complex<T> >& other) const
throw(std::bad_cast)
{
const EuclidianFourierMapComplex<T>& m2 = dynamic_cast<const EuclidianFourierMapComplex<T>&>(other);
if (this->size() != m2.size())
throw std::bad_cast();
const std::complex<T> *d1 = this->data();
const std::complex<T> *d2 = m2.data();
const DimArray& dims = this->getDims();
int N0 = dims[0] + (even0 ? 0 : 1);
std::complex<T> result = 0;
for (long q0 = 1; q0 < N0-1; q0++)
{
for (long p = 0; p < plane_size; p++)
{
long idx = q0+dims[0]*p;
assert(idx < this->size());
result += 2*(conj(d1[idx]) * d2[idx]).real();
}
}
if (even0)
{
for (long p = 0; p < plane_size; p++)
{
long q0 = N0*p, q1 = (p+1)*N0-1;
result += conj(d1[q0]) * d2[q0];
result += conj(d1[q1]) * d2[q1];
}
}
return result;
}
};
};
#endif

View File

@ -0,0 +1,215 @@
/*+
This is CosmoTool (./src/fourier/details/euclidian_spectrum_1d.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __DETAILS_EUCLIDIAN_SPECTRUM_1D
#define __DETAILS_EUCLIDIAN_SPECTRUM_1D
#include <iostream>
#include <boost/function.hpp>
namespace CosmoTool
{
template<typename T>
class EuclidianOperator
{
public:
typedef boost::function1<T, T> Function;
Function base, op;
T operator()(T k) {
return op(base(k));
}
};
template<typename T>
class EuclidianSpectrum_1D: public SpectrumFunction<T>
{
public:
typedef boost::function1<T, T> Function;
protected:
Function f;
static T msqrt(T a) { return std::sqrt(a); }
public:
typedef typename SpectrumFunction<T>::FourierMapType FourierMapType;
typedef typename SpectrumFunction<T>::SpectrumFunctionPtr SpectrumFunctionPtr;
typedef boost::shared_ptr<FourierMapType> ptr_map;
EuclidianSpectrum_1D(Function P)
: f(P)
{
}
void newRandomFourier(gsl_rng *rng, FourierMapType& out_map) const;
SpectrumFunctionPtr copy() const {
return SpectrumFunctionPtr(new EuclidianSpectrum_1D(f));
}
void sqrt() {
EuclidianOperator<T> o;
o.base = f;
o.op = &EuclidianSpectrum_1D<T>::msqrt;
f = (Function(o));
}
void mul(FourierMapType& m) const;
void mul_sqrt(FourierMapType& m) const;
void mul_inv(FourierMapType& m) const;
void mul_inv_sqrt(FourierMapType& m) const;
};
template<typename T>
void EuclidianSpectrum_1D<T>::newRandomFourier(gsl_rng *rng, FourierMapType& out_map) const
{
typedef EuclidianFourierMapComplex<T> MapT;
typedef typename EuclidianSpectrum_1D<T>::ptr_map ptr_map;
typedef typename MapT::DimArray DimArray;
MapT& rand_map = dynamic_cast<MapT&>(out_map);
std::complex<T> *d = rand_map.data();
long idx;
const DimArray& dims = rand_map.getDims();
const std::vector<double>& delta_k = rand_map.get_delta_k();
long plane_size;
bool alleven = rand_map.allDimensionsEven();
double V = 1;
for (int p = 0; p < delta_k.size(); p++)
V *= (2*M_PI/delta_k[p]);
for (long p = 1; p < rand_map.size(); p++)
{
double A_k = std::sqrt(0.5*V*f(rand_map.get_K(p)));
d[p] = std::complex<T>(gsl_ran_gaussian(rng, A_k),
gsl_ran_gaussian(rng, A_k));
}
// Generate the mean value
d[0] = std::complex<T>(gsl_ran_gaussian(rng, std::sqrt(V*f(0))), 0);
if (!rand_map.firstDimensionEven())
return;
// Correct the Nyquist plane
idx = dims[0]-1; // Stick to the last element of the first dimension
d[idx] = std::complex<T>(d[idx].real() + d[idx].imag(), 0);
// 1D is special case
if (dims.size() == 1)
return;
plane_size = 1;
for (int q = 1; q < dims.size(); q++)
{
plane_size *= dims[q];
}
for (long p = 1; p < plane_size/2; p++)
{
long q = (p+1)*dims[0]-1;
long q2 = (plane_size-p+1)*dims[0]-1;
assert(q < plane_size*dims[0]);
assert(q2 < plane_size*dims[0]);
d[q] = conj(d[q2]);
}
if (alleven)
{
long q = 0;
for (int i = dims.size()-1; i >= 1; i--)
q = dims[i]*q + dims[i]/2;
q += dims[0]-1;
d[q] = std::complex<T>(d[q].real()+d[q].imag(),0);
}
}
template<typename T>
void EuclidianSpectrum_1D<T>::mul(FourierMapType& m) const
{
EuclidianFourierMapComplex<T>& m_c = dynamic_cast<EuclidianFourierMapComplex<T>&>(m);
std::complex<T> *d = m.data();
for (long p = 0; p < m_c.size(); p++)
d[p] *= f(m_c.get_K(p));
}
template<typename T>
void EuclidianSpectrum_1D<T>::mul_sqrt(FourierMapType& m) const
{
EuclidianFourierMapComplex<T>& m_c = dynamic_cast<EuclidianFourierMapComplex<T>&>(m);
std::complex<T> *d = m.data();
for (long p = 0; p < m_c.size(); p++)
d[p] *= std::sqrt(f(m_c.get_K(p)));
}
template<typename T>
void EuclidianSpectrum_1D<T>::mul_inv(FourierMapType& m) const
{
EuclidianFourierMapComplex<T>& m_c = dynamic_cast<EuclidianFourierMapComplex<T>&>(m);
std::complex<T> *d = m.data();
for (long p = 0; p < m_c.size(); p++)
{
T A = f(m_c.get_K(p));
if (A==0)
d[p] = 0;
else
d[p] /= A;
}
}
template<typename T>
void EuclidianSpectrum_1D<T>::mul_inv_sqrt(FourierMapType& m) const
{
EuclidianFourierMapComplex<T>& m_c = dynamic_cast<EuclidianFourierMapComplex<T>&>(m);
std::complex<T> *d = m.data();
for (long p = 0; p < m_c.size(); p++)
{
T A = std::sqrt(f(m_c.get_K(p)));
if (A == 0)
d[p] = 0;
else
d[p] /= A;
}
}
};
#endif

View File

@ -0,0 +1,100 @@
/*+
This is CosmoTool (./src/fourier/details/euclidian_spectrum_1d_bin.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __DETAILS_EUCLIDIAN_SPECTRUM_1D_BIN
#define __DETAILS_EUCLIDIAN_SPECTRUM_1D_BIN
#include <boost/bind.hpp>
#include <cmath>
namespace CosmoTool
{
template<typename T>
class EuclidianSpectrum_1D_Binned: public EuclidianSpectrum_1D<T>
{
protected:
T *m_data;
long m_size;
T m_kmin, m_kmax, m_logdeltak;
std::vector<T> m_dof;
public:
typedef typename SpectrumFunction<T>::FourierMapType FourierMapType;
typedef typename SpectrumFunction<T>::SpectrumFunctionPtr SpectrumFunctionPtr;
typedef boost::shared_ptr<FourierMapType> ptr_map;
T interpolate_spectrum(T k)
{
T q = std::log(k/m_kmin)/m_logdeltak;
long ik = std::floor(q);
if (ik >= m_size-1)
return m_data[m_size-1];
else if (ik < 0)
return k/m_kmin*m_data[0];
return std::exp((q-ik)*m_data[ik+1] + (1-(q-ik))*m_data[ik]);
}
EuclidianSpectrum_1D_Binned(int numBin, T kmin, T kmax)
: EuclidianSpectrum_1D<T>(boost::bind(&EuclidianSpectrum_1D_Binned::interpolate_spectrum, this, _1))
{
m_data = new T[numBin];
m_kmin = kmin;
m_kmax = kmax;
m_size = numBin;
m_logdeltak = std::log(m_kmax/m_kmin);
}
SpectrumFunctionPtr copy() const
{
EuclidianSpectrum_1D_Binned *s = new EuclidianSpectrum_1D_Binned(m_size, m_kmin, m_kmax);
std::copy(m_data, m_data+m_size, s->m_data);
return SpectrumFunctionPtr(s);
}
void set_dof(std::vector<T>& dof_array)
{
assert(m_size == dof_array.size());
m_dof = dof_array;
}
const T *data() const { return m_data; }
long size() const { return m_size; }
const T *dof() const { return &m_dof[0]; }
};
};
#endif

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/*+
This is CosmoTool (./src/fourier/details/euclidian_transform.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __DETAILS_EUCLIDIAN_TRANSFORM
#define __DETAILS_EUCLIDIAN_TRANSFORM
namespace CosmoTool
{
template<typename T>
class EuclidianFourierTransform: public FourierTransform<T>
{
public:
typedef typename EuclidianFourierMapBase<T>::DimArray DimArray;
private:
typedef FFTW_Calls<T> calls;
EuclidianFourierMapReal<T> *realMap;
EuclidianFourierMapComplex<T> *fourierMap;
typename calls::plan_type m_analysis, m_synthesis;
double volume;
long N, Nc;
DimArray m_dims, m_dims_hc;
std::vector<double> m_L;
public:
EuclidianFourierTransform(const DimArray& dims, const std::vector<double>& L)
{
assert(L.size() == dims.size());
std::vector<double> dk(L.size());
std::vector<int> swapped_dims(dims.size());
m_dims = dims;
m_dims_hc = dims;
m_dims_hc[0] = dims[0]/2+1;
m_L = L;
N = 1;
Nc = 1;
volume = 1;
for (int i = 0; i < dims.size(); i++)
{
N *= dims[i];
Nc *= m_dims_hc[i];
volume *= L[i];
dk[i] = 2*M_PI/L[i];
swapped_dims[dims.size()-1-i] = dims[i];
}
realMap = new EuclidianFourierMapReal<T>(
boost::shared_ptr<T>(calls::alloc_real(N),
std::ptr_fun(calls::free)),
m_dims);
fourierMap = new EuclidianFourierMapComplex<T>(
boost::shared_ptr<std::complex<T> >((std::complex<T>*)calls::alloc_complex(Nc),
std::ptr_fun(calls::free)),
dims[0], m_dims_hc, dk);
m_analysis = calls::plan_dft_r2c(dims.size(), &swapped_dims[0],
realMap->data(), (typename calls::complex_type *)fourierMap->data(),
FFTW_DESTROY_INPUT|FFTW_MEASURE);
m_synthesis = calls::plan_dft_c2r(dims.size(), &swapped_dims[0],
(typename calls::complex_type *)fourierMap->data(), realMap->data(),
FFTW_DESTROY_INPUT|FFTW_MEASURE);
}
virtual ~EuclidianFourierTransform()
{
delete realMap;
delete fourierMap;
calls::destroy_plan(m_synthesis);
calls::destroy_plan(m_analysis);
}
void synthesis()
{
calls::execute(m_synthesis);
realMap->scale(1/volume);
}
void analysis()
{
calls::execute(m_analysis);
fourierMap->scale(volume/N);
}
void synthesis_conjugate()
{
calls::execute(m_analysis);
fourierMap->scale(1/volume);
}
void analysis_conjugate()
{
calls::execute(m_synthesis);
realMap->scale(volume/N);
}
const FourierMap<std::complex<T> >& fourierSpace() const
{
return *fourierMap;
}
FourierMap<std::complex<T> >& fourierSpace()
{
return *fourierMap;
}
const FourierMap<T>& realSpace() const
{
return *realMap;
}
FourierMap<T>& realSpace()
{
return *realMap;
}
FourierTransform<T> *mimick() const
{
return new EuclidianFourierTransform(m_dims, m_L);
}
};
template<typename T>
class EuclidianFourierTransform_1d: public EuclidianFourierTransform<T>
{
private:
template<typename T2>
static std::vector<T2> make_1d_vector(T2 a)
{
T2 arr[2] = { a};
return std::vector<T2>(&arr[0],&arr[1]);
}
public:
EuclidianFourierTransform_1d(int Nx, double Lx)
: EuclidianFourierTransform<T>(make_1d_vector<int>(Nx), make_1d_vector<double>(Lx))
{
}
virtual ~EuclidianFourierTransform_1d() {}
};
template<typename T>
class EuclidianFourierTransform_2d: public EuclidianFourierTransform<T>
{
private:
template<typename T2>
static std::vector<T2> make_2d_vector(T2 a, T2 b)
{
T2 arr[2] = { a, b};
return std::vector<T2>(&arr[0], &arr[2]);
}
public:
EuclidianFourierTransform_2d(int Nx, int Ny, double Lx, double Ly)
: EuclidianFourierTransform<T>(make_2d_vector<int>(Nx, Ny), make_2d_vector<double>(Lx, Ly))
{
}
virtual ~EuclidianFourierTransform_2d() {}
};
template<typename T>
class EuclidianFourierTransform_3d: public EuclidianFourierTransform<T>
{
private:
template<typename T2>
static std::vector<T2> make_3d_vector(T2 a, T2 b, T2 c)
{
T2 arr[3] = { a, b, c};
return std::vector<T2>(&arr[0], &arr[3]);
}
public:
EuclidianFourierTransform_3d(int Nx, int Ny, int Nz, double Lx, double Ly, double Lz)
: EuclidianFourierTransform<T>(make_3d_vector<int>(Nx, Ny, Nz), make_3d_vector<double>(Lx, Ly, Lz))
{
}
virtual ~EuclidianFourierTransform_3d() {}
};
};
#endif

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/*+
This is CosmoTool (./src/fourier/details/healpix_alms.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_FOURIER_HEALPIX_DETAILS_ALM_HPP
#define __COSMOTOOL_FOURIER_HEALPIX_DETAILS_ALM_HPP
namespace CosmoTool
{
template<typename T>
class HealpixFourierALM: public FourierMap<std::complex<T> >
{
private:
std::complex<T> *alms;
long m_size;
long Lmax_, Mmax_, TVal_;
Eigen::aligned_allocator<std::complex<T> > alloc;
public:
typedef unsigned long LType;
LType Lmax() const { return Lmax_; }
LType Mmax() const { return Mmax_; }
LType Num_Alms() const
{
return ((Mmax_+1)*(Mmax_+2))/2 + (Mmax_+1)*(Lmax_-Mmax_);
}
LType index_l0(LType m) const
{
return ((m*(TVal_-m))/2);
}
LType index(LType l, LType m) const
{
return index_l0(m) + l;
}
HealpixFourierALM(LType lmax, LType mmax)
: Lmax_(lmax), Mmax_(mmax), TVal_(2*lmax+1)
{
m_size = Num_Alms();
alms = alloc.allocate(m_size);
}
virtual ~HealpixFourierALM()
{
alloc.deallocate(alms, m_size);
}
virtual const std::complex<T>* data() const { return alms; }
virtual std::complex<T> * data() { return alms;}
virtual long size() const { return m_size; }
virtual FourierMap<std::complex<T> > *mimick() const
{
return new HealpixFourierALM<T>(Lmax_, Mmax_);
}
virtual std::complex<T> dot_product(const FourierMap<std::complex<T> >& other) const
throw(std::bad_cast)
{
const HealpixFourierALM<T>& mfm = dynamic_cast<const HealpixFourierALM<T>&>(other);
typedef typename FourierMap<std::complex<T> >::MapType MapType;
std::complex<T> S;
if (m_size != mfm.m_size)
throw std::bad_cast();
MapType m1(alms, m_size);
MapType m2(mfm.alms, mfm.m_size);
S = (m1.block(0,0,1,Lmax_+1).conjugate() * m2.block(0,0,1,Lmax_+1)).sum();
S += std::complex<T>(2,0)*(m1.block(0,1+Lmax_,1,m_size-1-Lmax_).conjugate() * m2.block(0,1+Lmax_,1,m_size-1-Lmax_)).sum();
return S;
}
};
};
#endif

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/*+
This is CosmoTool (./src/fourier/details/healpix_map.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_FOURIER_HEALPIX_DETAILS_MAP_HPP
#define __COSMOTOOL_FOURIER_HEALPIX_DETAILS_MAP_HPP
namespace CosmoTool
{
template<typename T>
class HealpixFourierMap: public FourierMap<T>
{
private:
T *m_data;
long Npix, m_Nside;
Eigen::aligned_allocator<T> alloc;
public:
HealpixFourierMap(long nSide)
: Npix(12*nSide*nSide), m_Nside(nSide)
{
m_data = alloc.allocate(Npix);
}
virtual ~HealpixFourierMap()
{
alloc.deallocate(m_data, Npix);
}
long Nside() const { return m_Nside; }
virtual const T* data() const { return m_data; }
virtual T *data() { return m_data; }
virtual long size() const { return Npix; }
virtual T dot_product(const FourierMap<T>& other) const
throw(std::bad_cast)
{
typedef typename FourierMap<T>::MapType MapType;
const HealpixFourierMap<T>& mfm = dynamic_cast<const HealpixFourierMap<T>&>(other);
if (Npix != mfm.size())
throw std::bad_cast();
MapType m1(m_data, Npix);
MapType m2(mfm.m_data, mfm.Npix);
return (m1*m2).sum();
}
virtual FourierMap<T> *mimick() const
{
return new HealpixFourierMap<T>(m_Nside);
}
};
};
#endif

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/*+
This is CosmoTool (./src/fourier/details/healpix_spectrum.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_FOURIER_HEALPIX_DETAILS_SPECTRUM_HPP
#define __COSMOTOOL_FOURIER_HEALPIX_DETAILS_SPECTRUM_HPP
namespace CosmoTool
{
template<typename T>
class HealpixSpectrum: public SpectrumFunction<T>
{
protected:
std::vector<T> cls;
int *m_dof;
public:
typedef typename SpectrumFunction<T>::FourierMapType FourierMapType;
typedef boost::shared_ptr<FourierMapType> ptr_map;
typedef typename SpectrumFunction<T>::SpectrumFunctionPtr SpectrumFunctionPtr;
typedef unsigned long LType;
HealpixSpectrum(LType Lmax)
: cls(Lmax+1), m_dof(new int[Lmax+1])
{
for (int l = 0; l <= Lmax; l++)
m_dof[l] = l + 1;
}
T *data() { return &cls[0]; }
const T *data() const { return &cls[0]; }
const int *dof() const { return m_dof; }
void set_dof(LType l, int dof) { m_dof[l] = dof; }
LType Lmax() const { return cls.size()-1; }
long size() const { return cls.size(); }
void newRandomFourier(gsl_rng *rng, FourierMapType& like_map) const;
SpectrumFunctionPtr copy() const {
HealpixSpectrum<T> *s = new HealpixSpectrum<T>(Lmax());
s->cls = cls;
return SpectrumFunctionPtr(s);
}
void sqrt() {
std::transform(cls.begin(), cls.end(), cls.begin(), std::ptr_fun<T,T>(std::sqrt));
}
void mul(FourierMapType& m) const;
void mul_sqrt(FourierMapType& m) const;
void mul_inv(FourierMapType& m) const;
void mul_inv_sqrt(FourierMapType& m) const;
};
template<typename T>
void HealpixSpectrum<T>::newRandomFourier(gsl_rng *rng, FourierMapType& out_map) const
{
HealpixFourierALM<T>& alms = dynamic_cast<HealpixFourierALM<T>&>(out_map);
long lmaxGen = std::min(cls.size()-1, alms.Lmax());
std::complex<T> *new_data = alms.data();
for (LType l = 0; l <= lmaxGen; l++)
{
double Al = std::sqrt(cls[l]);
new_data[alms.index(l,0)] = gsl_ran_gaussian(rng, Al);
Al *= M_SQRT1_2;
for (LType m = 1; m <= std::min(l,alms.Mmax()); m++)
{
std::complex<T>& c = new_data[alms.index(l,m)];
c.real() = gsl_ran_gaussian(rng, Al);
c.imag() = gsl_ran_gaussian(rng, Al);
}
}
}
template<typename T>
void HealpixSpectrum<T>::mul(FourierMapType& like_map) const
{
HealpixFourierALM<T>& alms = dynamic_cast<HealpixFourierALM<T>&>(like_map);
std::complex<T> *data = alms.data();
for (LType l = 0; l <= alms.Lmax(); l++)
{
double Al = cls[l];
for (LType m = 0; m <= std::min(l,alms.Mmax()); m++)
{
data[alms.index(l,m)] *= Al;
}
}
}
template<typename T>
void HealpixSpectrum<T>::mul_sqrt(FourierMapType& like_map) const
{
HealpixFourierALM<T>& alms = dynamic_cast<HealpixFourierALM<T>&>(like_map);
std::complex<T> *data = alms.data();
for (LType l = 0; l <= alms.Lmax(); l++)
{
double Al = std::sqrt(cls[l]);
for (LType m = 0; m <= std::min(l,alms.Mmax()); m++)
{
data[alms.index(l,m)] *= Al;
}
}
}
template<typename T>
void HealpixSpectrum<T>::mul_inv(FourierMapType& like_map) const
{
HealpixFourierALM<T>& alms = dynamic_cast<HealpixFourierALM<T>&>(like_map);
std::complex<T> *data = alms.data();
for (LType l = 0; l <= alms.Lmax(); l++)
{
double Al = (cls[l] <= 0) ? 0 : (1/cls[l]);
for (LType m = 0; m <= std::min(l,alms.Mmax()); m++)
{
data[alms.index(l,m)] *= Al;
}
}
}
template<typename T>
void HealpixSpectrum<T>::mul_inv_sqrt(FourierMapType& like_map) const
{
HealpixFourierALM<T>& alms = dynamic_cast<HealpixFourierALM<T>&>(like_map);
std::complex<T> *data = alms.data();
for (LType l = 0; l <= alms.Lmax(); l++)
{
double Al = (cls[l] <= 0) ? 0 : std::sqrt(1/cls[l]);
for (LType m = 0; m <= std::min(l,alms.Mmax()); m++)
{
data[alms.index(l,m)] *= Al;
}
}
}
};
#endif

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@ -0,0 +1,132 @@
/*+
This is CosmoTool (./src/fourier/details/healpix_transform.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_FOURIER_HEALPIX_DETAILS_TRANSFORM_HPP
#define __COSMOTOOL_FOURIER_HEALPIX_DETAILS_TRANSFORM_HPP
namespace CosmoTool
{
template<typename T> struct HealpixJobHelper__ {};
template<> struct HealpixJobHelper__<double>
{ enum {val=1}; };
template<> struct HealpixJobHelper__<float>
{ enum {val=0}; };
template<typename T>
class HealpixFourierTransform: public FourierTransform<T>
{
private:
sharp_alm_info *ainfo;
sharp_geom_info *ginfo;
HealpixFourierMap<T> realMap;
HealpixFourierALM<T> fourierMap;
int m_iterate;
public:
HealpixFourierTransform(long nSide, long Lmax, long Mmax, int iterate = 0)
: realMap(nSide), fourierMap(Lmax, Mmax), ainfo(0), ginfo(0), m_iterate(iterate)
{
sharp_make_healpix_geom_info (nSide, 1, &ginfo);
sharp_make_triangular_alm_info (Lmax, Mmax, 1, &ainfo);
}
virtual ~HealpixFourierTransform()
{
sharp_destroy_geom_info(ginfo);
sharp_destroy_alm_info(ainfo);
}
virtual const FourierMap<std::complex<T> >& fourierSpace() const { return fourierMap; }
virtual FourierMap<std::complex<T> >& fourierSpace() { return fourierMap; }
virtual const FourierMap<T>& realSpace() const { return realMap; }
virtual FourierMap<T>& realSpace() { return realMap; }
virtual FourierTransform<T> *mimick() const
{
return new HealpixFourierTransform<T>(realMap.Nside(), fourierMap.Lmax(), fourierMap.Mmax());
}
virtual void analysis()
{
void *aptr=reinterpret_cast<void *>(fourierMap.data()), *mptr=reinterpret_cast<void *>(realMap.data());
sharp_execute (SHARP_MAP2ALM, 0, 0, &aptr, &mptr, ginfo, ainfo, 1,
HealpixJobHelper__<T>::val,0,0,0);
for (int i = 0; i < m_iterate; i++)
{
HealpixFourierMap<T> tmp_map(realMap.Nside());
void *tmp_ptr=reinterpret_cast<void *>(tmp_map.data());
typename HealpixFourierMap<T>::MapType m0 = tmp_map.eigen();
typename HealpixFourierMap<T>::MapType m1 = realMap.eigen();
sharp_execute (SHARP_ALM2MAP, 0, 0, &aptr, &tmp_ptr, ginfo, ainfo, 1,
HealpixJobHelper__<T>::val,0,0,0);
m0 = m1 - m0;
sharp_execute (SHARP_MAP2ALM, 0, 1, &aptr, &tmp_ptr, ginfo, ainfo, 1,
HealpixJobHelper__<T>::val,0,0,0);
}
}
virtual void synthesis()
{
void *aptr=reinterpret_cast<void *>(fourierMap.data()), *mptr=reinterpret_cast<void *>(realMap.data());
sharp_execute (SHARP_ALM2MAP, 0, 0, &aptr, &mptr, ginfo, ainfo, 1,
HealpixJobHelper__<T>::val,0,0,0);
}
virtual void analysis_conjugate()
{
synthesis();
realMap.scale(4*M_PI/realMap.size());
}
virtual void synthesis_conjugate()
{
analysis();
fourierMap.scale(realMap.size()/(4*M_PI));
}
};
};
#endif

View File

@ -0,0 +1,98 @@
/*+
This is CosmoTool (./src/fourier/details/healpix_utility.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_FOURIER_HEALPIX_DETAILS_SPECTRUM_HP
#define __COSMOTOOL_FOURIER_HEALPIX_DETAILS_SPECTRUM_HP
namespace CosmoTool
{
template<typename T>
class HealpixUtilityFunction: public MapUtilityFunction<T>
{
public:
typedef typename MapUtilityFunction<T>::Spectrum Spectrum;
typedef typename MapUtilityFunction<T>::Spectrum_ptr Spectrum_ptr;
typedef typename MapUtilityFunction<T>::FMap FMap;
typedef typename HealpixSpectrum<T>::LType LType;
Spectrum_ptr estimateSpectrumFromMap(const FMap& m) const
{
const HealpixFourierALM<T>& alms = dynamic_cast<const HealpixFourierALM<T>&>(m);
LType Lmax = alms.Lmax(), Mmax = alms.Mmax();
HealpixSpectrum<T> *spectrum = new HealpixSpectrum<T>(Lmax);
T *data_cls = spectrum->data();
const std::complex<T> *data_alms = alms.data();
// make an estimate of the cls
std::fill(data_cls, data_cls+Lmax+1, 0);
LType q = 0;
for (LType m = 0; m <= Mmax; ++m )
{
for (LType l = m; l <= Lmax; ++l)
{
// Triangular storage
data_cls[l] += std::norm(data_alms[l+q]);
}
q += Lmax+1-m;
}
assert(q==alms.size());
for (LType l = 0; l <= Lmax; ++l)
{
int dof = 1 + std::min(l, Mmax);
spectrum->set_dof(l, dof);
data_cls[l] /= dof;
}
return Spectrum_ptr(spectrum);
}
Spectrum_ptr newSpectrumFromRaw(T *data, long size,
const Spectrum& like_spec) const
{
const HealpixSpectrum<T>& in_spec = dynamic_cast<const HealpixSpectrum<T>&>(like_spec);
HealpixSpectrum<T> *new_spectrum = new HealpixSpectrum<T>(in_spec.Lmax());
T *out_d = new_spectrum->data();
std::copy(data, data + min(size,new_spectrum->size()), out_d);
return Spectrum_ptr(new_spectrum);
}
};
};
#endif

View File

@ -1,6 +1,42 @@
/*+
This is CosmoTool (./src/fourier/euclidian.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_FOURIER_EUCLIDIAN_HPP #ifndef __COSMOTOOL_FOURIER_EUCLIDIAN_HPP
#define __COSMOTOOL_FOURIER_EUCLIDIAN_HPP #define __COSMOTOOL_FOURIER_EUCLIDIAN_HPP
#include <cmath>
#include <boost/function.hpp> #include <boost/function.hpp>
#include <vector> #include <vector>
#include <boost/shared_ptr.hpp> #include <boost/shared_ptr.hpp>
@ -8,400 +44,9 @@
#include "base_types.hpp" #include "base_types.hpp"
#include "fft/fftw_calls.hpp" #include "fft/fftw_calls.hpp"
#include "../algo.hpp" #include "../algo.hpp"
#include "details/euclidian_maps.hpp"
namespace CosmoTool #include "details/euclidian_spectrum_1d.hpp"
{ #include "details/euclidian_spectrum_1d_bin.hpp"
template<typename T> #include "details/euclidian_transform.hpp"
class EuclidianSpectrum_1D: public SpectrumFunction<T>
{
public:
typedef boost::function1<T, T> Function;
protected:
Function f;
public:
typedef typename SpectrumFunction<T>::FourierMapType FourierMapType;
typedef boost::shared_ptr<FourierMapType> ptr_map;
EuclidianSpectrum_1D(Function P)
: f(P)
{
}
ptr_map newRandomFourier(gsl_rng *rng, const FourierMapType& like_map) const;
void mul(FourierMap<std::complex<T> >& m) const;
};
template<typename T>
class EuclidianFourierMapBase: public FourierMap<T>
{
public:
typedef std::vector<int> DimArray;
private:
boost::shared_ptr<T> m_data;
DimArray m_dims;
long m_size;
public:
EuclidianFourierMapBase(boost::shared_ptr<T> indata, const DimArray& indims)
{
m_data = indata;
m_dims = indims;
m_size = 1;
for (int i = 0; i < m_dims.size(); i++)
m_size *= m_dims[i];
}
virtual ~EuclidianFourierMapBase()
{
}
const DimArray& getDims() const { return m_dims; }
virtual const T *data() const { return m_data.get(); }
virtual T *data() { return m_data.get(); }
virtual long size() const { return m_size; }
virtual FourierMap<T> *copy() const
{
FourierMap<T> *m = this->mimick();
m->eigen() = this->eigen();
return m;
}
};
template<typename T>
class EuclidianFourierMapReal: public EuclidianFourierMapBase<T>
{
public:
typedef typename EuclidianFourierMapBase<T>::DimArray DimArray;
EuclidianFourierMapReal(boost::shared_ptr<T> indata, const DimArray& indims)
: EuclidianFourierMapBase<T>(indata, indims)
{}
virtual FourierMap<T> *mimick() const
{
return new EuclidianFourierMapReal<T>(
boost::shared_ptr<T>((T *)fftw_malloc(sizeof(T)*this->size()),
std::ptr_fun(fftw_free)),
this->getDims());
}
virtual T dot_product(const FourierMap<T>& other) const
throw(std::bad_cast)
{
const EuclidianFourierMapReal<T>& m2 = dynamic_cast<const EuclidianFourierMapReal<T>&>(other);
if (this->size() != m2.size())
throw std::bad_cast();
return (this->eigen()*m2.eigen()).sum();
}
};
template<typename T>
class EuclidianFourierMapComplex: public EuclidianFourierMapBase<std::complex<T> >
{
protected:
typedef boost::shared_ptr<std::complex<T> > ptr_t;
std::vector<double> delta_k;
long plane_size;
public:
typedef typename EuclidianFourierMapBase<std::complex<T> >::DimArray DimArray;
EuclidianFourierMapComplex(ptr_t indata,
const DimArray& indims,
const std::vector<double>& dk)
: EuclidianFourierMapBase<std::complex<T> >(indata, indims), delta_k(dk)
{
assert(dk.size() == indims.size());
plane_size = 1;
for (int q = 1; q < indims.size(); q++)
plane_size *= indims[q];
}
virtual FourierMap<std::complex<T> > *mimick() const
{
return
new EuclidianFourierMapComplex<T>(
ptr_t((std::complex<T> *)
fftw_malloc(sizeof(std::complex<T>)*this->size()),
std::ptr_fun(fftw_free)),
this->getDims(),
this->delta_k);
}
template<typename Array>
double get_K(const Array& ik)
{
const DimArray& dims = this->getDims();
assert(ik.size() == dims.size());
double k2 = 0;
for (int q = 0; q < ik.size(); q++)
{
int dk = ik;
if (dk > dims[q]/2)
dk = dk - dims[q];
k2 += CosmoTool::square(delta_k[q]*dk);
}
return std::sqrt(k2);
}
double get_K(long p)
{
const DimArray& dims = this->getDims();
DimArray d(delta_k.size());
for (int q = 0; q < d.size(); q++)
{
d[q] = p%dims[q];
p = (p-d[q])/dims[q];
}
return get_K(d);
}
virtual std::complex<T> dot_product(const FourierMap<std::complex<T> >& other) const
throw(std::bad_cast)
{
const EuclidianFourierMapComplex<T>& m2 = dynamic_cast<const EuclidianFourierMapComplex<T>&>(other);
if (this->size() != m2.size())
throw std::bad_cast();
const std::complex<T> *d1 = this->data();
const std::complex<T> *d2 = m2.data();
const DimArray& dims = this->getDims();
int N0 = dims[0];
std::complex<T> result = 0;
for (long q0 = 1; q0 < N0-1; q0++)
{
for (long p = 0; p < plane_size; p++)
{
long idx = q0+N0*p;
assert(idx < this->size());
result += 2*(conj(d1[idx]) * d2[idx]).real();
}
}
for (long p = 0; p < plane_size; p++)
{
long q0 = N0*p, q1 = (p+1)*N0-1;
result += conj(d1[q0]) * d2[q0];
result += conj(d1[q1]) * d2[q1];
}
return result;
}
};
template<typename T>
class EuclidianFourierTransform: public FourierTransform<T>
{
public:
typedef typename EuclidianFourierMapBase<T>::DimArray DimArray;
private:
typedef FFTW_Calls<T> calls;
EuclidianFourierMapReal<T> *realMap;
EuclidianFourierMapComplex<T> *fourierMap;
typename calls::plan_type m_analysis, m_synthesis;
double volume;
long N;
DimArray m_dims, m_dims_hc;
std::vector<double> m_L;
public:
EuclidianFourierTransform(const DimArray& dims, const std::vector<double>& L)
{
assert(L.size() == dims.size());
std::vector<double> dk(L.size());
m_dims = dims;
m_dims_hc = dims;
m_dims_hc[0] = dims[0]/2+1;
m_L = L;
N = 1;
volume = 1;
for (int i = 0; i < dims.size(); i++)
{
N *= dims[i];
volume *= L[i];
dk[i] = 2*M_PI/L[i];
}
realMap = new EuclidianFourierMapReal<T>(
boost::shared_ptr<T>(calls::alloc_real(N),
std::ptr_fun(calls::free)),
m_dims);
fourierMap = new EuclidianFourierMapComplex<T>(
boost::shared_ptr<std::complex<T> >((std::complex<T>*)calls::alloc_complex(N),
std::ptr_fun(calls::free)),
m_dims_hc, dk);
m_analysis = calls::plan_dft_r2c(dims.size(), &dims[0],
realMap->data(), (typename calls::complex_type *)fourierMap->data(),
FFTW_MEASURE);
m_synthesis = calls::plan_dft_c2r(dims.size(), &dims[0],
(typename calls::complex_type *)fourierMap->data(), realMap->data(),
FFTW_MEASURE);
}
virtual ~EuclidianFourierTransform()
{
delete realMap;
delete fourierMap;
calls::destroy_plan(m_synthesis);
calls::destroy_plan(m_analysis);
}
void synthesis()
{
calls::execute(m_synthesis);
realMap->scale(1/volume);
}
void analysis()
{
calls::execute(m_analysis);
fourierMap->scale(volume/N);
}
void synthesis_conjugate()
{
calls::execute(m_analysis);
fourierMap->scale(1/volume);
}
void analysis_conjugate()
{
calls::execute(m_synthesis);
realMap->scale(volume/N);
}
const FourierMap<std::complex<T> >& fourierSpace() const
{
return *fourierMap;
}
FourierMap<std::complex<T> >& fourierSpace()
{
return *fourierMap;
}
const FourierMap<T>& realSpace() const
{
return *realMap;
}
FourierMap<T>& realSpace()
{
return *realMap;
}
FourierTransform<T> *mimick() const
{
return new EuclidianFourierTransform(m_dims, m_L);
}
};
template<typename T>
class EuclidianFourierTransform_2d: public EuclidianFourierTransform<T>
{
private:
template<typename T2>
static std::vector<T2> make_2d_vector(T2 a, T2 b)
{
T2 arr[2] = { a, b};
return std::vector<T2>(&arr[0], &arr[2]);
}
public:
EuclidianFourierTransform_2d(int Nx, int Ny, double Lx, double Ly)
: EuclidianFourierTransform<T>(make_2d_vector<int>(Nx, Ny), make_2d_vector<double>(Lx, Ly))
{
}
virtual ~EuclidianFourierTransform_2d() {}
};
template<typename T>
class EuclidianFourierTransform_3d: public EuclidianFourierTransform<T>
{
private:
template<typename T2>
static std::vector<T2> make_3d_vector(T2 a, T2 b, T2 c)
{
T2 arr[2] = { a, b, c};
return std::vector<T2>(&arr[0], &arr[3]);
}
public:
EuclidianFourierTransform_3d(int Nx, int Ny, int Nz, double Lx, double Ly, double Lz)
: EuclidianFourierTransform<T>(make_3d_vector<int>(Nx, Ny, Nz), make_3d_vector<double>(Lx, Ly, Lz))
{
}
virtual ~EuclidianFourierTransform_3d() {}
};
template<typename T>
typename EuclidianSpectrum_1D<T>::ptr_map
EuclidianSpectrum_1D<T>::newRandomFourier(gsl_rng *rng, const FourierMapType& like_map) const
{
typedef EuclidianFourierMapComplex<T> MapT;
typedef typename MapT::DimArray DimArray;
MapT& m_c = dynamic_cast<MapT&>(like_map);
MapT *rand_map = m_c.mimick();
std::complex<T> *d = rand_map->data();
long idx;
const DimArray& dims = rand_map->getDims();
long plane_size;
for (long p = 1; p < m_c.size(); p++)
{
double A_k = std::sqrt(0.5*f(rand_map->get_K(p)));
d[p] = std::complex<T>(gsl_ran_gaussian(rng, A_k),
gsl_ran_gaussian(rng, A_k));
}
// Generate the mean value
d[0] = std::complex<T>(std::sqrt(f(0)), 0);
// Correct the Nyquist plane
idx = dims[0]-1; // Stick to the last element of the first dimension
// 1D is special case
if (dims.size() == 1)
{
d[idx] = std::complex<T>(d[idx].real() + d[idx].imag(), 0);
return boost::shared_ptr<EuclidianSpectrum_1D<T>::FourierMapType>(rand_map);
}
plane_size = 1;
for (int q = 1; q < dims.size(); q++)
{
plane_size *= dims[q];
}
for (long p = 1; p < plane_size/2; p++)
{
long q = (p+1)*dims[0]-1;
long q2 = (plane_size-p+1)*dims[0]-1;
assert(q < plane_size*dims[0]);
assert(q2 < plane_size*dims[0]);
d[q] = conj(d[q2]);
}
long q = dims[0];
d[q] = std::complex<T>(d[q].real() + d[q].imag());
}
template<typename T>
void EuclidianSpectrum_1D<T>::mul(FourierMap<std::complex<T> >& m) const
{
EuclidianFourierMapComplex<T>& m_c = dynamic_cast<EuclidianFourierMapComplex<T>&>(m);
std::complex<T> *d = m.data();
for (long p = 0; p < m_c.size(); p++)
d[p] *= f(m.get_K(p));
}
};
#endif #endif

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/fourier/fft/fftw_calls.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __FFTW_UNIFIED_CALLS_HPP #ifndef __FFTW_UNIFIED_CALLS_HPP
#define __FFTW_UNIFIED_CALLS_HPP #define __FFTW_UNIFIED_CALLS_HPP
@ -28,8 +63,8 @@ public: \
typedef prefix ## _complex complex_type; \ typedef prefix ## _complex complex_type; \
typedef prefix ## _plan plan_type; \ typedef prefix ## _plan plan_type; \
\ \
static complex_type *alloc_complex(int N) { return prefix ## _alloc_complex(N); } \ static complex_type *alloc_complex(size_t N) { return prefix ## _alloc_complex(N); } \
static real_type *alloc_real(int N) { return prefix ## _alloc_real(N); } \ static real_type *alloc_real(size_t N) { return prefix ## _alloc_real(N); } \
static void free(void *p) { fftw_free(p); } \ static void free(void *p) { fftw_free(p); } \
\ \
static void execute(plan_type p) { prefix ## _execute(p); } \ static void execute(plan_type p) { prefix ## _execute(p); } \

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/fourier/healpix.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_FOURIER_HEALPIX_HPP #ifndef __COSMOTOOL_FOURIER_HEALPIX_HPP
#define __COSMOTOOL_FOURIER_HEALPIX_HPP #define __COSMOTOOL_FOURIER_HEALPIX_HPP
@ -12,257 +47,13 @@
#include <sharp_lowlevel.h> #include <sharp_lowlevel.h>
#include <sharp_geomhelpers.h> #include <sharp_geomhelpers.h>
#include <sharp_almhelpers.h> #include <sharp_almhelpers.h>
#include <algorithm>
#include <functional>
namespace CosmoTool #include "details/healpix_map.hpp"
{ #include "details/healpix_alms.hpp"
template<typename T> #include "details/healpix_transform.hpp"
class HealpixSpectrum: public SpectrumFunction<T> #include "details/healpix_spectrum.hpp"
{ #include "details/healpix_utility.hpp"
protected:
std::vector<T> cls;
public:
typedef typename SpectrumFunction<T>::FourierMapType FourierMapType;
typedef boost::shared_ptr<FourierMapType> ptr_map;
HealpixSpectrum(long Lmax)
: cls(Lmax+1) {}
T *data() { return &cls[0]; }
const T *data() const { return &cls[0]; }
long size() const { return cls.size(); }
ptr_map newRandomFourier(gsl_rng *rng, const FourierMapType& like_map) const = 0;
};
template<typename T>
class HealpixFourierMap: public FourierMap<T>
{
private:
T *m_data;
long Npix, m_Nside;
Eigen::aligned_allocator<T> alloc;
public:
HealpixFourierMap(long nSide)
: Npix(12*nSide*nSide), m_Nside(nSide)
{
m_data = alloc.allocate(Npix);
}
virtual ~HealpixFourierMap()
{
alloc.deallocate(m_data, Npix);
}
long Nside() const { return m_Nside; }
virtual const T* data() const { return m_data; }
virtual T *data() { return m_data; }
virtual long size() const { return Npix; }
virtual T dot_product(const FourierMap<T>& other) const
throw(std::bad_cast)
{
typedef typename FourierMap<T>::MapType MapType;
const HealpixFourierMap<T>& mfm = dynamic_cast<const HealpixFourierMap<T>&>(other);
if (Npix != mfm.size())
throw std::bad_cast();
MapType m1(m_data, Npix);
MapType m2(mfm.m_data, mfm.Npix);
return (m1*m2).sum();
}
virtual FourierMap<T> *mimick() const
{
return new HealpixFourierMap<T>(m_Nside);
}
};
template<typename T>
class HealpixFourierALM: public FourierMap<std::complex<T> >
{
private:
std::complex<T> *alms;
long m_size;
long Lmax_, Mmax_, TVal_;
Eigen::aligned_allocator<std::complex<T> > alloc;
public:
typedef unsigned long LType;
LType Lmax() const { return Lmax_; }
LType Mmax() const { return Mmax_; }
LType Num_Alms() const
{
return ((Mmax_+1)*(Mmax_+2))/2 + (Mmax_+1)*(Lmax_-Mmax_);
}
LType index_l0(LType m) const
{
return ((m*(TVal_-m))/2);
}
LType index(LType l, LType m) const
{
return index_l0(m) + l;
}
HealpixFourierALM(LType lmax, LType mmax)
: Lmax_(lmax), Mmax_(mmax), TVal_(2*lmax+1)
{
m_size = Num_Alms();
alms = alloc.allocate(m_size);
}
virtual ~HealpixFourierALM()
{
alloc.deallocate(alms, m_size);
}
virtual const std::complex<T>* data() const { return alms; }
virtual std::complex<T> * data() { return alms;}
virtual long size() const { return m_size; }
virtual FourierMap<std::complex<T> > *mimick() const
{
return new HealpixFourierALM<T>(Lmax_, Mmax_);
}
virtual std::complex<T> dot_product(const FourierMap<std::complex<T> >& other) const
throw(std::bad_cast)
{
const HealpixFourierALM<T>& mfm = dynamic_cast<const HealpixFourierALM<T>&>(other);
typedef typename FourierMap<std::complex<T> >::MapType MapType;
std::complex<T> S;
if (m_size != mfm.m_size)
throw std::bad_cast();
MapType m1(alms, m_size);
MapType m2(mfm.alms, mfm.m_size);
S = (m1.block(0,0,1,Lmax_+1).conjugate() * m2.block(0,0,1,Lmax_+1)).sum();
S += std::complex<T>(2,0)*(m1.block(0,1+Lmax_,1,m_size-1-Lmax_).conjugate() * m2.block(0,1+Lmax_,1,m_size-1-Lmax_)).sum();
return S;
}
};
template<typename T> struct HealpixJobHelper__ {};
template<> struct HealpixJobHelper__<double>
{ enum {val=1}; };
template<> struct HealpixJobHelper__<float>
{ enum {val=0}; };
template<typename T>
class HealpixFourierTransform: public FourierTransform<T>
{
private:
sharp_alm_info *ainfo;
sharp_geom_info *ginfo;
HealpixFourierMap<T> realMap;
HealpixFourierALM<T> fourierMap;
int m_iterate;
public:
HealpixFourierTransform(long nSide, long Lmax, long Mmax, int iterate = 0)
: realMap(nSide), fourierMap(Lmax, Mmax), ainfo(0), ginfo(0), m_iterate(iterate)
{
sharp_make_healpix_geom_info (nSide, 1, &ginfo);
sharp_make_triangular_alm_info (Lmax, Mmax, 1, &ainfo);
}
virtual ~HealpixFourierTransform()
{
sharp_destroy_geom_info(ginfo);
sharp_destroy_alm_info(ainfo);
}
virtual const FourierMap<std::complex<T> >& fourierSpace() const { return fourierMap; }
virtual FourierMap<std::complex<T> >& fourierSpace() { return fourierMap; }
virtual const FourierMap<T>& realSpace() const { return realMap; }
virtual FourierMap<T>& realSpace() { return realMap; }
virtual FourierTransform<T> *mimick() const
{
return new HealpixFourierTransform<T>(realMap.Nside(), fourierMap.Lmax(), fourierMap.Mmax());
}
virtual void analysis()
{
void *aptr=reinterpret_cast<void *>(fourierMap.data()), *mptr=reinterpret_cast<void *>(realMap.data());
sharp_execute (SHARP_MAP2ALM, 0, 0, &aptr, &mptr, ginfo, ainfo, 1,
HealpixJobHelper__<T>::val,0,0,0);
for (int i = 0; i < m_iterate; i++)
{
HealpixFourierMap<T> tmp_map(realMap.Nside());
void *tmp_ptr=reinterpret_cast<void *>(tmp_map.data());
typename HealpixFourierMap<T>::MapType m0 = tmp_map.eigen();
typename HealpixFourierMap<T>::MapType m1 = realMap.eigen();
sharp_execute (SHARP_ALM2MAP, 0, 0, &aptr, &tmp_ptr, ginfo, ainfo, 1,
HealpixJobHelper__<T>::val,0,0,0);
m0 = m1 - m0;
sharp_execute (SHARP_MAP2ALM, 0, 1, &aptr, &tmp_ptr, ginfo, ainfo, 1,
HealpixJobHelper__<T>::val,0,0,0);
}
}
virtual void synthesis()
{
void *aptr=reinterpret_cast<void *>(fourierMap.data()), *mptr=reinterpret_cast<void *>(realMap.data());
sharp_execute (SHARP_ALM2MAP, 0, 0, &aptr, &mptr, ginfo, ainfo, 1,
HealpixJobHelper__<T>::val,0,0,0);
}
virtual void analysis_conjugate()
{
synthesis();
realMap.scale(4*M_PI/realMap.size());
}
virtual void synthesis_conjugate()
{
analysis();
fourierMap.scale(realMap.size()/(4*M_PI));
}
};
template<typename T>
typename HealpixSpectrum<T>::ptr_map
HealpixSpectrum<T>::newRandomFourier(gsl_rng *rng, const FourierMapType& like_map) const
{
const HealpixFourierALM<T>& alms = dynamic_cast<const HealpixFourierALM<T>&>(like_map);
HealpixFourierALM<T> *new_alms;
ptr_map r(new_alms = new HealpixFourierALM<T>(alms.Lmax(), alms.Mmax()));
long lmaxGen = std::min(cls.size()-1, alms.Lmax());
std::complex<T> *new_data = new_alms->data();
for (long l = 0; l < lmaxGen; l++)
{
double Al = std::sqrt(cls[l]);
new_data[alms.index(l,0)] = gsl_ran_gaussian(rng, Al);
Al *= M_SQRT1_2;
for (long m = 1; m < alms.Mmax(); m++)
{
std::complex<T>& c = new_data[alms.index(l,m)];
c.real() = gsl_ran_gaussian(rng, Al);
c.imag() = gsl_ran_gaussian(rng, Al);
}
}
return r;
}
};
#endif #endif

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/growthFactor.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <cmath> #include <cmath>
#include <gsl/gsl_integration.h> #include <gsl/gsl_integration.h>
#include "interpolate.hpp" #include "interpolate.hpp"

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/growthFactor.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef COSMO_GROWTH_FACTOR_HPP #ifndef COSMO_GROWTH_FACTOR_HPP
#define COSMO_GROWTH_FACTOR_HPP #define COSMO_GROWTH_FACTOR_HPP

View File

@ -1,3 +1,11 @@
/*+
!!
This file has been developped by P. M. Sutter
!!
+*/
/* This file contains the functions that read the data from the HDF5 file /* This file contains the functions that read the data from the HDF5 file
* The functions accept the PARAMESH data through arguments. * The functions accept the PARAMESH data through arguments.
*/ */
@ -185,7 +193,7 @@ void h5_read_flash3_particles (H5File* file,
float *vel1, float *vel1,
float *vel2, float *vel2,
float *vel3, float *vel3,
int *id) long *id)
{ {
herr_t status; herr_t status;
@ -341,7 +349,7 @@ void h5_read_flash3_particles (H5File* file,
if (id) { if (id) {
for(p=0; p < (pcount); p++) { for(p=0; p < (pcount); p++) {
id[p+poffset] = (int) *(partBuffer+iptag-1+p*numProps); id[p+poffset] = (long) *(partBuffer+iptag-1+p*numProps);
} } } }
if (pos1 && pos2 && pos3) { if (pos1 && pos2 && pos3) {

View File

@ -1,3 +1,12 @@
/*+
!!! NOTE !!!
This file has been developped by P. M. Sutter.
!!!!
+*/
/* This file contains the functions that read the data from the HDF5 file /* This file contains the functions that read the data from the HDF5 file
* The functions accept the PARAMESH data through arguments. * The functions accept the PARAMESH data through arguments.
*/ */
@ -29,7 +38,7 @@ void h5_read_flash3_particles (H5File* file,
float *vel1, float *vel1,
float *vel2, float *vel2,
float *vel3, float *vel3,
int *id); long *id);
void h5_read_flash3_header_info(H5File* file, void h5_read_flash3_header_info(H5File* file,
double* time, /* simulation time */ double* time, /* simulation time */

View File

@ -1,3 +1,10 @@
/*+
!!
This particular file has been developped by P. M. Sutter
!!
+*/
/* general header file for the HDF 5 IO in FLASH */ /* general header file for the HDF 5 IO in FLASH */

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/interpolate.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <cassert> #include <cassert>
#include <cmath> #include <cmath>
#include <algorithm> #include <algorithm>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/interpolate.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __CTOOL_INTERPOLATE_HPP #ifndef __CTOOL_INTERPOLATE_HPP
#define __CTOOL_INTERPOLATE_HPP #define __CTOOL_INTERPOLATE_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/interpolate3d.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMO_INTERPOLATE3D_HPP #ifndef __COSMO_INTERPOLATE3D_HPP
#define __COSMO_INTERPOLATE3D_HPP #define __COSMO_INTERPOLATE3D_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/kdtree_leaf.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __LEAF_KDTREE_HPP #ifndef __LEAF_KDTREE_HPP
#define __LEAF_KDTREE_HPP #define __LEAF_KDTREE_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/kdtree_splitters.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __KDTREE_SPLITTERS_HPP #ifndef __KDTREE_SPLITTERS_HPP
#define __KDTREE_SPLITTERS_HPP #define __KDTREE_SPLITTERS_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/loadFlash.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
/* Reads in FLASH v3 files in HDF5 format */ /* Reads in FLASH v3 files in HDF5 format */
#include <iostream> #include <iostream>
@ -71,7 +106,7 @@ SimuData *CosmoTool::loadFlashMulti(const char *fname, int id, int loadflags)
} } } }
if (loadflags & NEED_GADGET_ID) { if (loadflags & NEED_GADGET_ID) {
data->Id = new int[data->NumPart]; data->Id = new long[data->NumPart];
if (data->Id == 0) { if (data->Id == 0) {
delete data; delete data;
return 0; return 0;

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/loadFlash.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMO_LOAD_FLASH_HPP #ifndef __COSMO_LOAD_FLASH_HPP
#define __COSMO_LOAD_FLASH_HPP #define __COSMO_LOAD_FLASH_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/loadFlash_dummy.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include "load_data.hpp" #include "load_data.hpp"
#include "loadFlash.hpp" #include "loadFlash.hpp"

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/loadGadget.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <cmath> #include <cmath>
#include <iostream> #include <iostream>
#include <assert.h> #include <assert.h>
@ -10,61 +45,41 @@
using namespace CosmoTool; using namespace CosmoTool;
using namespace std; using namespace std;
PurePositionData *CosmoTool::loadGadgetPosition(const char *fname)
{
PurePositionData *data;
int p, n;
UnformattedRead f(fname);
GadgetHeader h;
data = new PurePositionData;
f.beginCheckpoint();
for (int i = 0; i < 6; i++)
h.npart[i] = f.readInt32();
for (int i = 0; i < 6; i++)
h.mass[i] = f.readReal64();
h.time = f.readReal64();
h.redshift = f.readReal64();
h.flag_sfr = f.readInt32();
h.flag_feedback = f.readInt32();
for (int i = 0; i < 6; i++)
h.npartTotal[i] = f.readInt32();
h.flag_cooling = f.readInt32();
h.num_files = f.readInt32();
data->BoxSize = h.BoxSize = f.readReal64();
h.Omega0 = f.readReal64();
h.OmegaLambda = f.readReal64();
h.HubbleParam = f.readReal64();
f.endCheckpoint(true);
data->NumPart = 0;
for(int k=0; k<5; k++)
data->NumPart += h.npart[k];
data->pos = new FCoordinates[data->NumPart];
f.beginCheckpoint();
for(int k = 0, p = 0; k < 5; k++) {
for(int n = 0; n < h.npart[k]; n++) {
data->pos[p][0] = f.readReal32();
data->pos[p][1] = f.readReal32();
data->pos[p][2] = f.readReal32();
p++;
}
}
f.endCheckpoint();
// Skip velocities
f.skip((long)data->NumPart*3+2*4);
// Skip ids
return data; void loadGadgetHeader(UnformattedRead *f, GadgetHeader& h, SimuData *data, int id)
{
f->beginCheckpoint();
for (int i = 0; i < 6; i++)
h.npart[i] = f->readInt32();
for (int i = 0; i < 6; i++)
h.mass[i] = f->readReal64();
data->time = h.time = f->readReal64();
h.redshift = f->readReal64();
h.flag_sfr = f->readInt32();
h.flag_feedback = f->readInt32();
for (int i = 0; i < 6; i++)
h.npartTotal[i] = f->readInt32();
h.flag_cooling = f->readInt32();
h.num_files = f->readInt32();
data->BoxSize = h.BoxSize = f->readReal64();
data->Omega_M = h.Omega0 = f->readReal64();
data->Omega_Lambda = h.OmegaLambda = f->readReal64();
data->Hubble = h.HubbleParam = f->readReal64();
f->endCheckpoint(true);
long NumPart = 0, NumPartTotal = 0;
for(int k=0; k<6; k++)
{
NumPart += h.npart[k];
NumPartTotal += (id < 0) ? h.npart[k] : h.npartTotal[k];
}
data->NumPart = NumPart;
data->TotalNumPart = NumPartTotal;
} }
SimuData *CosmoTool::loadGadgetMulti(const char *fname, int id,
int loadflags, int GadgetFormat,
SimuFilter filter)
SimuData *CosmoTool::loadGadgetMulti(const char *fname, int id, int loadflags, int GadgetFormat)
{ {
SimuData *data; SimuData *data;
int p, n; int p, n;
@ -98,35 +113,11 @@ SimuData *CosmoTool::loadGadgetMulti(const char *fname, int id, int loadflags, i
} }
long NumPart = 0, NumPartTotal = 0; long NumPart = 0, NumPartTotal = 0;
try try
{ {
f->beginCheckpoint(); loadGadgetHeader(f, h, data, id);
for (int i = 0; i < 6; i++)
h.npart[i] = f->readInt32();
for (int i = 0; i < 6; i++)
h.mass[i] = f->readReal64();
data->time = h.time = f->readReal64();
h.redshift = f->readReal64();
h.flag_sfr = f->readInt32();
h.flag_feedback = f->readInt32();
for (int i = 0; i < 6; i++)
h.npartTotal[i] = f->readInt32();
h.flag_cooling = f->readInt32();
h.num_files = f->readInt32();
data->BoxSize = h.BoxSize = f->readReal64();
data->Omega_M = h.Omega0 = f->readReal64();
data->Omega_Lambda = h.OmegaLambda = f->readReal64();
data->Hubble = h.HubbleParam = f->readReal64();
f->endCheckpoint(true);
for(int k=0; k<6; k++)
{
NumPart += h.npart[k];
NumPartTotal += (id < 0) ? h.npart[k] : h.npartTotal[k];
}
data->NumPart = NumPart;
data->TotalNumPart = NumPartTotal;
if (GadgetFormat == 1) if (GadgetFormat == 1)
velmul = sqrt(h.time); velmul = sqrt(h.time);
else if (GadgetFormat == 2) else if (GadgetFormat == 2)
@ -135,6 +126,9 @@ SimuData *CosmoTool::loadGadgetMulti(const char *fname, int id, int loadflags, i
cerr << "unknown gadget format" << endl; cerr << "unknown gadget format" << endl;
abort(); abort();
} }
NumPart = data->NumPart;
NumPartTotal = data->TotalNumPart;
} }
catch (const InvalidUnformattedAccess& e) catch (const InvalidUnformattedAccess& e)
{ {
@ -236,7 +230,7 @@ SimuData *CosmoTool::loadGadgetMulti(const char *fname, int id, int loadflags, i
try try
{ {
f->beginCheckpoint(); f->beginCheckpoint();
data->Id = new int[data->NumPart]; data->Id = new long[data->NumPart];
if (data->Id == 0) if (data->Id == 0)
{ {
delete f; delete f;

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/loadGadget.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMO_LOAD_GADGET_HPP #ifndef __COSMO_LOAD_GADGET_HPP
#define __COSMO_LOAD_GADGET_HPP #define __COSMO_LOAD_GADGET_HPP
@ -7,10 +42,9 @@
#include "loadSimu.hpp" #include "loadSimu.hpp"
namespace CosmoTool { namespace CosmoTool {
PurePositionData *loadGadgetPosition(const char *fname);
SimuData *loadGadgetMulti(const char *fname, int id, int flags, int GadgetFormat = 1); SimuData *loadGadgetMulti(const char *fname, int id, int flags,
int GadgetFormat = 1, SimuFilter filter = 0);
// Only single snapshot supported // Only single snapshot supported
void writeGadget(const std::string& fname, SimuData *data, int GadgetFormat = 1); void writeGadget(const std::string& fname, SimuData *data, int GadgetFormat = 1);

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/loadRamses.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <sys/types.h> #include <sys/types.h>
#include <regex.h> #include <regex.h>
#include <cmath> #include <cmath>
@ -318,6 +353,9 @@ CosmoTool::SimuData *CosmoTool::loadRamsesSimu(const char *basename, int outputI
data->Omega_M = info.omega_m; data->Omega_M = info.omega_m;
data->Omega_Lambda = info.omega_lambda; data->Omega_Lambda = info.omega_lambda;
if (flags == 0)
return data;
if (cpuid < 0) if (cpuid < 0)
cpuid = 1; cpuid = 1;
else cpuid++; else cpuid++;
@ -381,7 +419,7 @@ CosmoTool::SimuData *CosmoTool::loadRamsesSimu(const char *basename, int outputI
} }
if (flags & NEED_GADGET_ID) if (flags & NEED_GADGET_ID)
{ {
data->Id = new int[nPar]; data->Id = new long[nPar];
} }
for (int k = 0; k < 3; k++) for (int k = 0; k < 3; k++)

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/loadRamses.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef _LOAD_RAMSES_HPP #ifndef _LOAD_RAMSES_HPP
#define _LOAD_RAMSES_HPP #define _LOAD_RAMSES_HPP

View File

@ -1,6 +1,43 @@
/*+
This is CosmoTool (./src/loadSimu.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOLBOX_HPP #ifndef __COSMOTOOLBOX_HPP
#define __COSMOTOOLBOX_HPP #define __COSMOTOOLBOX_HPP
#include <map>
#include <string>
namespace CosmoTool namespace CosmoTool
{ {
@ -9,9 +46,24 @@ namespace CosmoTool
static const int NEED_VELOCITY = 4; static const int NEED_VELOCITY = 4;
static const int NEED_TYPE = 8; static const int NEED_TYPE = 8;
struct SimuParticle
{
float Pos[3];
float Vel[3];
int type;
int id;
bool flag_vel, flag_type, flag_id;
};
typedef bool (*SimuFilter)(const SimuParticle& p);
class SimuData class SimuData
{ {
public: public:
typedef void (*FreeFunction)(void *);
typedef std::map<std::string, std::pair<void *, FreeFunction> > AttributeMap;
float BoxSize; float BoxSize;
float time; float time;
float Hubble; float Hubble;
@ -21,10 +73,13 @@ namespace CosmoTool
long NumPart; long NumPart;
long TotalNumPart; long TotalNumPart;
int *Id; long *Id;
float *Pos[3]; float *Pos[3];
float *Vel[3]; float *Vel[3];
int *type; int *type;
AttributeMap attributes;
public: public:
SimuData() : Id(0),NumPart(0),type(0) { Pos[0]=Pos[1]=Pos[2]=0; Vel[0]=Vel[1]=Vel[2]=0; } SimuData() : Id(0),NumPart(0),type(0) { Pos[0]=Pos[1]=Pos[2]=0; Vel[0]=Vel[1]=Vel[2]=0; }
~SimuData() ~SimuData()
@ -40,7 +95,37 @@ namespace CosmoTool
delete[] type; delete[] type;
if (Id) if (Id)
delete[] Id; delete[] Id;
for (AttributeMap::iterator i = attributes.begin();
i != attributes.end();
++i)
{
if (i->second.second)
i->second.second(i->second.first);
}
} }
template<typename T>
T *as(const std::string& n)
{
AttributeMap::iterator i = attributes.find(n);
if (i == attributes.end())
return 0;
return reinterpret_cast<T *>(i->second.first);
}
void new_attribute(const std::string& n, void *p, FreeFunction free_func)
{
AttributeMap::iterator i = attributes.find(n);
if (i != attributes.end())
{
if (i->second.second)
i->second.second(i->second.first);
}
attributes[n] = std::make_pair(p, free_func);
}
}; };
}; };

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/load_data.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <assert.h> #include <assert.h>
#include <stdio.h> #include <stdio.h>
#include <stdlib.h> #include <stdlib.h>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/load_data.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef _LOAD_GADGET_DATA_HPP #ifndef _LOAD_GADGET_DATA_HPP
#define _LOAD_GADGET_DATA_HPP #define _LOAD_GADGET_DATA_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/mach.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMO_MACHINE_TEST_HPP #ifndef __COSMO_MACHINE_TEST_HPP
#define __COSMO_MACHINE_TEST_HPP #define __COSMO_MACHINE_TEST_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/miniargs.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <cstdlib> #include <cstdlib>
#include <cstdio> #include <cstdio>
#include <cstring> #include <cstring>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/miniargs.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef _MAK_MINIARGS_HPP #ifndef _MAK_MINIARGS_HPP
#define _MAK_MINIARGS_HPP #define _MAK_MINIARGS_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/mykdtree.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __HV_KDTREE_HPP #ifndef __HV_KDTREE_HPP
#define __HV_KDTREE_HPP #define __HV_KDTREE_HPP
@ -65,15 +100,16 @@ namespace CosmoTool {
class RecursionMultipleInfo class RecursionMultipleInfo
{ {
public: public:
const typename KDDef<N,CType>::KDCoordinates& x; typename KDDef<N,CType>::KDCoordinates x;
BoundedQueue< KDCell<N,ValType,CType> *, typename KDDef<N,CType>::CoordType> queue; BoundedQueue< KDCell<N,ValType,CType> *, typename KDDef<N,CType>::CoordType> queue;
int traversed; int traversed;
RecursionMultipleInfo(const typename KDDef<N,CType>::KDCoordinates& rx, RecursionMultipleInfo(const typename KDDef<N,CType>::KDCoordinates& rx,
KDCell<N,ValType,CType> **cells, KDCell<N,ValType,CType> **cells,
uint32_t numCells) uint32_t numCells)
: x(rx), queue(cells, numCells, INFINITY),traversed(0) : queue(cells, numCells, INFINITY),traversed(0)
{ {
std::copy(rx, rx+N, x);
} }
}; };
@ -97,6 +133,12 @@ namespace CosmoTool {
KDTree(Cell *cells, uint32_t Ncells); KDTree(Cell *cells, uint32_t Ncells);
~KDTree(); ~KDTree();
void setPeriodic(bool on, CoordType replicate)
{
periodic = on;
this->replicate = replicate;
}
uint32_t getIntersection(const coords& x, CoordType r, uint32_t getIntersection(const coords& x, CoordType r,
Cell **cells, Cell **cells,
uint32_t numCells) uint32_t numCells)
@ -150,6 +192,9 @@ namespace CosmoTool {
Cell **sortingHelper; Cell **sortingHelper;
Cell *base_cell; Cell *base_cell;
bool periodic;
CoordType replicate;
Node *buildTree(Cell **cell0, Node *buildTree(Cell **cell0,
uint32_t NumCells, uint32_t NumCells,
uint32_t depth, uint32_t depth,

View File

@ -1,3 +1,4 @@
#include "replicateGenerator.hpp"
#include <cstring> #include <cstring>
#include <algorithm> #include <algorithm>
#include <limits> #include <limits>
@ -31,7 +32,8 @@ namespace CosmoTool {
template<int N, typename ValType, typename CType, typename CellSplitter> template<int N, typename ValType, typename CType, typename CellSplitter>
KDTree<N,ValType,CType,CellSplitter>::KDTree(Cell *cells, uint32_t Ncells) KDTree<N,ValType,CType,CellSplitter>::KDTree(Cell *cells, uint32_t Ncells)
{ {
periodic = false;
base_cell = cells; base_cell = cells;
numNodes = Ncells; numNodes = Ncells;
nodes = new Node[numNodes]; nodes = new Node[numNodes];
@ -93,6 +95,19 @@ namespace CosmoTool {
info.distances = 0; info.distances = 0;
recursiveIntersectionCells<false>(info, root, 0); recursiveIntersectionCells<false>(info, root, 0);
if (periodic)
{
ReplicateGenerator<float, N> r(x, replicate);
do
{
coords x_new;
r.getPosition(info.x);
recursiveIntersectionCells<false>(info, root, 0);
}
while (r.next());
}
return info.currentRank; return info.currentRank;
} }
@ -114,6 +129,18 @@ namespace CosmoTool {
info.distances = distances; info.distances = distances;
recursiveIntersectionCells<false>(info, root, 0); recursiveIntersectionCells<false>(info, root, 0);
if (periodic)
{
ReplicateGenerator<float, N> r(x, replicate);
do
{
coords x_new;
r.getPosition(info.x);
recursiveIntersectionCells<false>(info, root, 0);
}
while (r.next());
}
return info.currentRank; return info.currentRank;
} }
@ -131,6 +158,19 @@ namespace CosmoTool {
info.distances = 0; info.distances = 0;
recursiveIntersectionCells<true>(info, root, 0); recursiveIntersectionCells<true>(info, root, 0);
if (periodic)
{
ReplicateGenerator<float, N> r(x, replicate);
do
{
coords x_new;
r.getPosition(info.x);
recursiveIntersectionCells<true>(info, root, 0);
}
while (r.next());
}
return info.currentRank; return info.currentRank;
} }
@ -365,7 +405,19 @@ namespace CosmoTool {
CoordType R2 = INFINITY; CoordType R2 = INFINITY;
Cell *best = 0; Cell *best = 0;
recursiveNearest(root, 0, x, R2, best); recursiveNearest(root, 0, x, R2, best);
if (periodic)
{
ReplicateGenerator<float, N> r(x, replicate);
do
{
coords x_new;
r.getPosition(x_new);
recursiveNearest(root, 0, x_new, R2, best);
}
while (r.next());
}
return best; return best;
} }
@ -437,6 +489,18 @@ namespace CosmoTool {
cells[i] = 0; cells[i] = 0;
recursiveMultipleNearest(info, root, 0); recursiveMultipleNearest(info, root, 0);
if (periodic)
{
ReplicateGenerator<float, N> r(x, replicate);
do
{
coords x_new;
r.getPosition(info.x);
recursiveMultipleNearest(info, root, 0);
}
while (r.next());
}
// std::cout << "Traversed = " << info.traversed << std::endl; // std::cout << "Traversed = " << info.traversed << std::endl;
} }
@ -452,9 +516,19 @@ namespace CosmoTool {
cells[i] = 0; cells[i] = 0;
recursiveMultipleNearest(info, root, 0); recursiveMultipleNearest(info, root, 0);
memcpy(distances, info.queue.getPriorities(), sizeof(CoordType)*N2); if (periodic)
{
ReplicateGenerator<float, N> r(x, replicate);
// std::cout << "Traversed = " << info.traversed << std::endl; do
{
coords x_new;
r.getPosition(info.x);
recursiveMultipleNearest(info, root, 0);
}
while (r.next());
}
memcpy(distances, info.queue.getPriorities(), sizeof(CoordType)*N2);
} }
#ifdef __KD_TREE_SAVE_ON_DISK #ifdef __KD_TREE_SAVE_ON_DISK

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/newton.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef _COSMOTOOL_NEWTON_HPP #ifndef _COSMOTOOL_NEWTON_HPP
#define _COSMOTOOL_NEWTON_HPP #define _COSMOTOOL_NEWTON_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/octTree.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <iostream> #include <iostream>
#include <cmath> #include <cmath>
#include <cassert> #include <cassert>

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/octTree.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_AMR_HPP #ifndef __COSMOTOOL_AMR_HPP
#define __COSMOTOOL_AMR_HPP #define __COSMOTOOL_AMR_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/pool.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMO_POOL_HPP #ifndef __COSMO_POOL_HPP
#define __COSMO_POOL_HPP #define __COSMO_POOL_HPP

View File

@ -1,3 +1,39 @@
/*+
This is CosmoTool (./src/powerSpectrum.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include <cassert>
#include <vector> #include <vector>
#include <algorithm> #include <algorithm>
#include <iostream> #include <iostream>
@ -21,7 +57,7 @@ using namespace std;
#define POWER_BDM 7 #define POWER_BDM 7
#define POWER_TEST 8 #define POWER_TEST 8
#define POWER_SPECTRUM HU_WIGGLES #define POWER_SPECTRUM POWER_EFSTATHIOU
namespace Cosmology { namespace Cosmology {
@ -651,4 +687,17 @@ double computeCorrel2(double powNorm, double topHatRad1, double topHatRad2)
#endif #endif
} }
double vvCorrection(double P_deltadelta, double k)
{
static const double alpha0 = -12480.5, alpha1 = 1.824, alpha2 = 2165.87, alpha3=1.796;
if (k > 0.3)
return 0;
double r =(alpha0*sqrt(P_deltadelta) + alpha1*P_deltadelta*P_deltadelta)/(alpha2 + alpha3*P_deltadelta);
assert(P_deltadelta > 0);
if (r < 0)
return 0;
return r;
}
}; };

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/powerSpectrum.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef _POWERSPECTRUM_HPP #ifndef _POWERSPECTRUM_HPP
#define _POWERSPECTRUM_HPP #define _POWERSPECTRUM_HPP
@ -30,6 +65,8 @@ namespace Cosmology {
double computeVarianceZero(double powNorm); double computeVarianceZero(double powNorm);
double computeCorrel(double powNorm, double topHatRad1); double computeCorrel(double powNorm, double topHatRad1);
double computeCorrel2(double powNorm, double topHatRad1, double topHatRad2); double computeCorrel2(double powNorm, double topHatRad1, double topHatRad2);
double vvCorrection(double P_deltadelta, double k);
}; };
#endif #endif

100
src/replicateGenerator.hpp Normal file
View File

@ -0,0 +1,100 @@
/*+
This is CosmoTool (./src/replicateGenerator.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __REPLICATE_GENERATOR_HPP
#define __REPLICATE_GENERATOR_HPP
#include <algorithm>
#include "algo.hpp"
namespace CosmoTool
{
template<typename Coord, int N>
class ReplicateGenerator
{
public:
typedef Coord Coords[N];
Coord replicate;
ReplicateGenerator(const Coords& x, Coord shift)
{
face = 0;
replicate = shift;
numFaces = spower<N,long>(3);
std::copy(x, x+N, x_base);
if (!next())
abort();
}
bool next()
{
if (face == numFaces)
return false;
face++;
bool no_move = true;
int q_face = face;
for (int i = 0; i < N; i++)
{
int c_face;
c_face = q_face % 3;
q_face /= 3;
x_shifted[i] = x_base[i] + (c_face-1)*replicate;
no_move = no_move && (c_face == 1);
}
if (no_move)
return next();
return true;
}
const Coord *getPosition()
{
return x_shifted;
}
void getPosition(Coords& x_out)
{
std::copy(x_shifted, x_shifted+N, x_out);
}
private:
Coord x_shifted[N], x_base[N];
long face, numFaces;
};
};
#endif

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/sparseGrid.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __VOID_SPARSE_GRID_HPP #ifndef __VOID_SPARSE_GRID_HPP
#define __VOID_SPARSE_GRID_HPP #define __VOID_SPARSE_GRID_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/sphSmooth.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __COSMOTOOL_SPH_SMOOTH_HPP #ifndef __COSMOTOOL_SPH_SMOOTH_HPP
#define __COSMOTOOL_SPH_SMOOTH_HPP #define __COSMOTOOL_SPH_SMOOTH_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/yorick.hpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#ifndef __YORICK_HELPERS_HPP #ifndef __YORICK_HELPERS_HPP
#define __YORICK_HELPERS_HPP #define __YORICK_HELPERS_HPP

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/yorick_nc3.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include "ctool_netcdf_ver.hpp" #include "ctool_netcdf_ver.hpp"
#include "config.hpp" #include "config.hpp"
#ifdef NETCDFCPP4 #ifdef NETCDFCPP4
@ -151,7 +186,7 @@ namespace CosmoTool {
ProgressiveOutput<T>::saveArrayProgressive(const std::string& fname, uint32_t *dimList, ProgressiveOutput<T>::saveArrayProgressive(const std::string& fname, uint32_t *dimList,
uint32_t rank) uint32_t rank)
{ {
NcFile *f = new NcFile(fname.c_str(), NcFile::Replace); NcFile *f = new NcFile(fname.c_str(), NcFile::Replace, 0, 0, NcFile::Netcdf4);
assert(f->is_valid()); assert(f->is_valid());
@ -202,7 +237,7 @@ namespace CosmoTool {
void saveArray(const std::string& fname, void saveArray(const std::string& fname,
T *array, uint32_t *dimList, uint32_t rank) T *array, uint32_t *dimList, uint32_t rank)
{ {
NcFile f(fname.c_str(), NcFile::Replace); NcFile f(fname.c_str(), NcFile::Replace, 0, 0, NcFile::Netcdf4);
assert(f.is_valid()); assert(f.is_valid());

View File

@ -1,3 +1,38 @@
/*+
This is CosmoTool (./src/yorick_nc4.cpp) -- Copyright (C) Guilhem Lavaux (2007-2013)
guilhem.lavaux@gmail.com
This software is a computer program whose purpose is to provide a toolbox for cosmological
data analysis (e.g. filters, generalized Fourier transforms, power spectra, ...)
This software is governed by the CeCILL license under French law and
abiding by the rules of distribution of free software. You can use,
modify and/ or redistribute the software under the terms of the CeCILL
license as circulated by CEA, CNRS and INRIA at the following URL
"http://www.cecill.info".
As a counterpart to the access to the source code and rights to copy,
modify and redistribute granted by the license, users are provided only
with a limited warranty and the software's author, the holder of the
economic rights, and the successive licensors have only limited
liability.
In this respect, the user's attention is drawn to the risks associated
with loading, using, modifying and/or developing or reproducing the
software by the user in light of its specific status of free software,
that may mean that it is complicated to manipulate, and that also
therefore means that it is reserved for developers and experienced
professionals having in-depth computer knowledge. Users are therefore
encouraged to load and test the software's suitability as regards their
requirements in conditions enabling the security of their systems and/or
data to be ensured and, more generally, to use and operate it in the
same conditions as regards security.
The fact that you are presently reading this means that you have had
knowledge of the CeCILL license and that you accept its terms.
+*/
#include "ctool_netcdf_ver.hpp" #include "ctool_netcdf_ver.hpp"
#include "config.hpp" #include "config.hpp"
#include <netcdf> #include <netcdf>