Power spectrum stuff (#16)

* add autok1d

* update TODO

* add basic cross pk

* del blank line

* fix small bugs

* fix loop bug

* rm nbs

* edit docstring

* Update TODO

* get rid of verbose flag

* take all ICs

* attempt better memory

* simplify ASCII dump

* rm verbose statement to get rid of bugs!

* close fortran files

* add MAS options

* add boxsize setter

* Move comment up

* paths chagne

* Update TODO

* Update TODO

* Forgotten units in Xpk

* Attempt at fixing the distance bug

* Update TODO

* Update TODO

* Remove comment

* add summary reader

* Update gitignore
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Richard Stiskalek 2022-12-12 14:42:44 +00:00 committed by GitHub
parent 1bb4255874
commit c3c686fa60
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10 changed files with 439 additions and 5314 deletions

1
.gitignore vendored
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@ -17,3 +17,4 @@ csiborgtools.egg-info/*
scripts/playground_* scripts/playground_*
scripts/*.ipynb scripts/*.ipynb
Pylians3/* Pylians3/*
scripts/plot_correlation.ipynb

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@ -1,20 +1,27 @@
# CSiBORG tools # CSiBORG tools
## Questions to answer
- How well can observed clusters be matched to CSiBORG? Do their masses agree?
- Is the number of clusters in CSiBORG consistent?
- Are any observed clusters suspiciously missing in CSiBORG?
## Short-term TODO ## Short-term TODO
- [ ] Get `powmes` working and compare its power spectrum to `Pylians`. - [x] Add code to calculate the cross-correlation for resolved region only.
- [ ] Check alignment of the angular momentum - [ ] Calculate the spectra for all 101 boxes and visualise them.
- [x] Make sure I am not taking halos outside of the well-resolved region. - [ ] See about the $z=70$ particles.
- [x] Calculate the gravitational potential.
- [x] Add the gravitational field calculation.
## Long-term TODO ## Long-term TODO
- [ ] Calculate the cross-correlation in CSiBORG. Should see the scale of the constraints? - [ ] Calculate the cross-correlation in CSiBORG. Should see the scale of the constraints?
- [ ] Find the distribution of particles in the first snapshot - [ ] Find the distribution of particles in the first snapshot
- [ ] Implement a custom model for matchin galaxies to halos. - [ ] Implement a custom model for matchin galaxies to halos.
- [x] Calculate DM environmental properties.
## Open questions ## Open questions
- What scaling of the search region? No reason for it to be a multiple of $R_{200c}$. - What scaling of the search region? No reason for it to be a multiple of $R_{200c}$.
- Begin extracting the DM environmental properties at galaxy positions? - Begin extracting the DM environmental properties at galaxy positions?
## Notes
- New sims with part files in initial snapshot: `/mnt/extraspace/hdesmond/ramses_out_7468_new`. Also numbers 7588, 8020, 8452, 8836.

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@ -12,9 +12,12 @@
# You should have received a copy of the GNU General Public License along # You should have received a copy of the GNU General Public License along
# with this program; if not, write to the Free Software Foundation, Inc., # with this program; if not, write to the Free Software Foundation, Inc.,
# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA. # 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
"""
Density field and cross-correlation calculations.
"""
import numpy import numpy
import MAS_library as MASL import MAS_library as MASL
import Pk_library as PKL
import smoothing_library as SL import smoothing_library as SL
from warnings import warn from warnings import warn
from tqdm import trange from tqdm import trange
@ -22,15 +25,24 @@ from ..units import (BoxUnits, radec_to_cartesian)
class DensityField: class DensityField:
""" r"""
Density field calculations. Based primarily on routines of Pylians [1]. Density field calculations. Based primarily on routines of Pylians [1].
Parameters Parameters
---------- ----------
particles : structured array particles : structured array
Particle array. Must contain keys `['x', 'y', 'z', 'M']`. Particle array. Must contain keys `['x', 'y', 'z', 'M']`. Particle
coordinates are assumed to be :math:`\in [0, 1]` or in box units
otherwise.
boxsize : float
Box length. Multiplies `particles` positions to fix the power spectum
units.
box : :py:class:`csiborgtools.units.BoxUnits` box : :py:class:`csiborgtools.units.BoxUnits`
The simulation box information and transformations. The simulation box information and transformations.
MAS : str, optional
Mass assignment scheme. Options are Options are: 'NGP' (nearest grid
point), 'CIC' (cloud-in-cell), 'TSC' (triangular-shape cloud), 'PCS'
(piecewise cubic spline).
References References
---------- ----------
@ -39,11 +51,13 @@ class DensityField:
_particles = None _particles = None
_boxsize = None _boxsize = None
_box = None _box = None
_MAS = None
def __init__(self, particles, box): def __init__(self, particles, boxsize, box, MAS="CIC"):
self.particles = particles self.particles = particles
self.box = box self.box = box
self._boxsize = 1. self.boxsize = boxsize
self.MAS = MAS
@property @property
def particles(self): def particles(self):
@ -64,6 +78,22 @@ class DensityField:
"containing `['x', 'y', 'z', 'M']`.") "containing `['x', 'y', 'z', 'M']`.")
self._particles = particles self._particles = particles
@property
def boxsize(self):
"""
Box length. Determines the power spectrum units.
Returns
-------
boxsize : float
"""
return self._boxsize
@boxsize.setter
def boxsize(self, boxsize):
"""Set `self.boxsize`."""
self._boxsize = boxsize
@property @property
def box(self): def box(self):
""" """
@ -83,15 +113,24 @@ class DensityField:
self._box = box self._box = box
@property @property
def boxsize(self): def MAS(self):
""" """
Boxsize. The mass-assignment scheme.
Returns Returns
------- -------
boxsize : float MAS : str
""" """
return self._boxsize return self._MAS
@MAS.setter
def MAS(self, MAS):
"""Sets `self.MAS`."""
opts = ["NGP", "CIC", "TSC", "PCS"]
if MAS not in opts:
raise ValueError("Invalid MAS `{}`. Options are: `{}`."
.format(MAS, opts))
self._MAS = MAS
@staticmethod @staticmethod
def _force_f32(x, name): def _force_f32(x, name):
@ -127,11 +166,10 @@ class DensityField:
pos *= self.boxsize pos *= self.boxsize
pos = self._force_f32(pos, "pos") pos = self._force_f32(pos, "pos")
weights = self._force_f32(self.particles['M'], 'M') weights = self._force_f32(self.particles['M'], 'M')
MAS = "CIC" # Cloud in cell
# Pre-allocate and do calculations # Pre-allocate and do calculations
rho = numpy.zeros((grid, grid, grid), dtype=numpy.float32) rho = numpy.zeros((grid, grid, grid), dtype=numpy.float32)
MASL.MA(pos, rho, self.boxsize, MAS, W=weights, verbose=verbose) MASL.MA(pos, rho, self.boxsize, self.MAS, W=weights, verbose=verbose)
return rho return rho
def overdensity_field(self, grid, verbose=True): def overdensity_field(self, grid, verbose=True):
@ -176,7 +214,8 @@ class DensityField:
delta = self.overdensity_field(grid, verbose) delta = self.overdensity_field(grid, verbose)
if verbose: if verbose:
print("Calculating potential from the overdensity..") print("Calculating potential from the overdensity..")
return MASL.potential(delta, self.box._omega_m, self.box._aexp, "CIC") return MASL.potential(
delta, self.box._omega_m, self.box._aexp, self.MAS)
def tensor_field(self, grid, verbose=True): def tensor_field(self, grid, verbose=True):
""" """
@ -196,8 +235,8 @@ class DensityField:
the relevant tensor components. the relevant tensor components.
""" """
delta = self.overdensity_field(grid, verbose) delta = self.overdensity_field(grid, verbose)
return MASL.tidal_tensor(delta, self.box._omega_m, self.box._aexp, return MASL.tidal_tensor(
"CIC") delta, self.box._omega_m, self.box._aexp, self.MAS)
def gravitational_field(self, grid, verbose=True): def gravitational_field(self, grid, verbose=True):
""" """
@ -219,7 +258,28 @@ class DensityField:
""" """
delta = self.overdensity_field(grid, verbose) delta = self.overdensity_field(grid, verbose)
return MASL.grav_field_tensor( return MASL.grav_field_tensor(
delta, self.box._omega_m, self.box._aexp, "CIC") delta, self.box._omega_m, self.box._aexp, self.MAS)
def auto_powerspectrum(self, grid, verbose=True):
"""
Calculate the auto 1-dimensional power spectrum.
Parameters
----------
grid : int
The grid size.
verbose : float, optional
A verbosity flag. By default `True`.
Returns
-------
pk : py:class`Pk_library.Pk`
Power spectrum object.
"""
delta = self.overdensity_field(grid, verbose)
return PKL.Pk(
delta, self.boxsize, axis=1, MAS=self.MAS, threads=1,
verbose=verbose)
def smooth_field(self, field, scale, threads=1): def smooth_field(self, field, scale, threads=1):
""" """

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@ -18,3 +18,4 @@ from .make_cat import (HaloCatalogue, CombinedHaloCatalogue) # noqa
from .readobs import (PlanckClusters, MCXCClusters, TwoMPPGalaxies, # noqa from .readobs import (PlanckClusters, MCXCClusters, TwoMPPGalaxies, # noqa
TwoMPPGroups, SDSS) # noqa TwoMPPGroups, SDSS) # noqa
from .outsim import (dump_split, combine_splits, make_ascii_powmes) # noqa from .outsim import (dump_split, combine_splits, make_ascii_powmes) # noqa
from .summaries import PKReader # noqa

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@ -18,11 +18,9 @@ I/O functions for analysing the CSiBORG realisations.
import numpy import numpy
from os.path import (join, dirname, basename, isfile) from os.path import (join, isfile)
import gc
from os import remove from os import remove
from tqdm import trange from tqdm import trange
from astropy.io import ascii
from astropy.table import Table from astropy.table import Table
I64 = numpy.int64 I64 = numpy.int64
@ -125,10 +123,9 @@ def combine_splits(n_splits, part_reader, cols_add, remove_splits=False,
return out return out
def make_ascii_powmes(particles, fout, verbose=True): def make_ascii_powmes(particles, fout):
""" """
Write an ASCII file with appropriate formatting for POWMES. Write an ASCII file with appropriate formatting for POWMES.
This is an extremely memory inefficient implementation.
Parameters Parameters
---------- ----------
@ -136,8 +133,6 @@ def make_ascii_powmes(particles, fout, verbose=True):
Array of particles. Array of particles.
fout : str fout : str
File path to store the ASCII file. File path to store the ASCII file.
verbose : bool, optional
Verbosity flag. By default `True`.
Returns Returns
------- -------
@ -146,27 +141,11 @@ def make_ascii_powmes(particles, fout, verbose=True):
out = Table() out = Table()
for p in ('x', 'y', 'z', 'M'): for p in ('x', 'y', 'z', 'M'):
out[p] = particles[p] out[p] = particles[p]
Npart = particles.size
# If fout exists, remove # If fout exists, remove
if isfile(fout): if isfile(fout):
remove(fout) remove(fout)
# Write the temporaty file with open(fout, 'wb') as f:
ftemp = join(dirname(fout), "_" + basename(fout)) numpy.savetxt(f, out, delimiter=',', header=str(Npart), comments='')
if verbose:
print("Writing temporary file `{}`...".format(ftemp))
ascii.write(out, ftemp, overwrite=True, delimiter=",", fast_writer=True)
del out
gc.collect()
# Write to the first line the number of particles
if verbose:
print("Writing the full file `{}`...".format(fout))
with open(ftemp, 'r') as fread, open(fout, 'w') as fwrite:
fwrite.write(str(particles.size) + '\n')
for i, line in enumerate(fread):
if i == 0:
continue
fwrite.write(line)
remove(ftemp)

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@ -249,6 +249,8 @@ class CSiBORGPaths:
files = [f.split("/")[-1] for f in files] files = [f.split("/")[-1] for f in files]
# Remove files with inverted ICs # Remove files with inverted ICs
files = [f for f in files if "_inv" not in f] files = [f for f in files if "_inv" not in f]
# Remove the new files with z = 70 only
files = [f for f in files if "_new" not in f]
# Remove the filename with _old # Remove the filename with _old
files = [f for f in files if "OLD" not in f] files = [f for f in files if "OLD" not in f]
ids = [int(f.split("_")[-1]) for f in files] ids = [int(f.split("_")[-1]) for f in files]
@ -596,6 +598,9 @@ class ParticleReader:
out[fname][i:i + j] = self.read_sp(fdtype, partfiles[cpu]) out[fname][i:i + j] = self.read_sp(fdtype, partfiles[cpu])
else: else:
dum[i:i + j] = self.read_sp(fdtype, partfiles[cpu]) dum[i:i + j] = self.read_sp(fdtype, partfiles[cpu])
# Close the fortran files
for partfile in partfiles:
partfile.close()
return out return out
@ -645,6 +650,8 @@ class ParticleReader:
j = nparts[cpu] j = nparts[cpu]
ff = self.open_unbinding(cpu) ff = self.open_unbinding(cpu)
clumpid[i:i + j] = ff.read_ints() clumpid[i:i + j] = ff.read_ints()
# Close
ff.close()
return clumpid return clumpid

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@ -0,0 +1,168 @@
# Copyright (C) 2022 Richard Stiskalek, Harry Desmond
# This program is free software; you can redistribute it and/or modify it
# under the terms of the GNU General Public License as published by the
# Free Software Foundation; either version 3 of the License, or (at your
# option) any later version.
#
# This program is distributed in the hope that it will be useful, but
# WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General
# Public License for more details.
#
# You should have received a copy of the GNU General Public License along
# with this program; if not, write to the Free Software Foundation, Inc.,
# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
"""
Tools for summarising various results.
"""
import numpy
import joblib
from tqdm import tqdm
class PKReader:
"""
A shortcut object for reading in the power spectrum files.
Parameters
----------
ic_ids : list of int
IC IDs to be read.
hw : float
Box half-width.
fskel : str, optional
The skeleton path. By default
`/mnt/extraspace/rstiskalek/csiborg/crosspk/out_{}_{}_{}.p`, where
the formatting options are `ic0, ic1, hw`.
dtype : dtype, optional
Output precision. By default `numpy.float32`.
"""
def __init__(self, ic_ids, hw, fskel=None, dtype=numpy.float32):
self.ic_ids = ic_ids
self.hw = hw
if fskel is None:
fskel = "/mnt/extraspace/rstiskalek/csiborg/crosspk/out_{}_{}_{}.p"
self.fskel = fskel
self.dtype = dtype
@staticmethod
def _set_klim(kmin, kmax):
"""
Sets limits on the wavenumber to 0 and infinity if `None`s provided.
"""
if kmin is None:
kmin = 0
if kmax is None:
kmax = numpy.infty
return kmin, kmax
def read_autos(self, kmin=None, kmax=None):
"""
Read in the autocorrelation power spectra.
Parameters
----------
kmin : float, optional
The minimum wavenumber. By default `None`, i.e. 0.
kmin : float, optional
The maximum wavenumber. By default `None`, i.e. infinity.
Returns
-------
ks : 1-dimensional array
Array of wavenumbers.
pks : 2-dimensional array of shape `(len(self.ic_ids), ks.size)`
Autocorrelation of each simulation.
"""
kmin, kmax = self._set_klim(kmin, kmax)
ks, pks, sel = None, None, None
for i, nsim in enumerate(self.ic_ids):
pk = joblib.load(self.fskel.format(nsim, nsim, self.hw))
# Get cuts and pre-allocate arrays
if i == 0:
x = pk.k3D
sel = (kmin < x) & (x < kmax)
ks = x[sel].astype(self.dtype)
pks = numpy.full((len(self.ic_ids), numpy.sum(sel)), numpy.nan,
dtype=self.dtype)
pks[i, :] = pk.Pk[sel, 0, 0]
return ks, pks
def read_single_cross(self, ic0, ic1, kmin=None, kmax=None):
"""
Read cross-correlation between IC IDs `ic0` and `ic1`.
Parameters
----------
ic0 : int
The first IC ID.
ic1 : int
The second IC ID.
kmin : float, optional
The minimum wavenumber. By default `None`, i.e. 0.
kmin : float, optional
The maximum wavenumber. By default `None`, i.e. infinity.
Returns
-------
ks : 1-dimensional array
Array of wavenumbers.
xpk : 1-dimensional array of shape `(ks.size, )`
Cross-correlation.
"""
if ic0 == ic1:
raise ValueError("Requested cross correlation for the same ICs.")
kmin, kmax = self._set_klim(kmin, kmax)
# Check their ordering. The latter must be larger.
ics = (ic0, ic1)
if ic0 > ic1:
ics = ics[::-1]
pk = joblib.load(self.fskel.format(*ics, self.hw))
ks = pk.k3D
sel = (kmin < ks) & (ks < kmax)
ks = ks[sel].astype(self.dtype)
xpk = pk.XPk[sel, 0, 0].astype(self.dtype)
return ks, xpk
def read_cross(self, kmin=None, kmax=None):
"""
Read cross-correlation between all IC pairs.
Parameters
----------
kmin : float, optional
The minimum wavenumber. By default `None`, i.e. 0.
kmin : float, optional
The maximum wavenumber. By default `None`, i.e. infinity.
Returns
-------
ks : 1-dimensional array
Array of wavenumbers.
xpks : 3-dimensional array of shape (`nics, nics - 1, ks.size`)
Cross-correlations. The first column is the the IC and is being
cross-correlated with the remaining ICs, in the second column.
"""
nics = len(self.ic_ids)
ks, xpks = None, None
for i, ic0 in enumerate(tqdm(self.ic_ids)):
k = 0
for ic1 in self.ic_ids:
# We don't want cross-correlation
if ic0 == ic1:
continue
x, y = self.read_single_cross(ic0, ic1, kmin, kmax)
# If in the first iteration pre-allocate arrays
if ks is None:
ks = x
xpks = numpy.full((nics, nics - 1, ks.size), numpy.nan,
dtype=self.dtype)
xpks[i, k, :] = y
# Bump up the iterator
k += 1
return ks, xpks

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scripts/run_crosspk.py Normal file
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@ -0,0 +1,168 @@
# Copyright (C) 2022 Richard Stiskalek
# This program is free software; you can redistribute it and/or modify it
# under the terms of the GNU General Public License as published by the
# Free Software Foundation; either version 3 of the License, or (at your
# option) any later version.
#
# This program is distributed in the hope that it will be useful, but
# WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General
# Public License for more details.
#
# You should have received a copy of the GNU General Public License along
# with this program; if not, write to the Free Software Foundation, Inc.,
# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
"""
MPI script to calculate the matter cross power spectrum between CSiBORG
IC realisations. Units are Mpc/h.
"""
from argparse import ArgumentParser
import numpy
import joblib
from datetime import datetime
from itertools import combinations
from os.path import join
from os import remove
from gc import collect
from mpi4py import MPI
import Pk_library as PKL
try:
import csiborgtools
except ModuleNotFoundError:
import sys
sys.path.append("../")
import csiborgtools
import utils
parser = ArgumentParser()
parser.add_argument("--grid", type=int)
parser.add_argument("--halfwidth", type=float, default=0.5)
args = parser.parse_args()
# Get MPI things
comm = MPI.COMM_WORLD
rank = comm.Get_rank()
nproc = comm.Get_size()
MAS = "CIC" # mass asignment scheme
paths = csiborgtools.read.CSiBORGPaths()
ics = paths.ic_ids
n_sims = len(ics)
# File paths
ftemp = join(utils.dumpdir, "temp_crosspk",
"out_{}_{}" + "_{}".format(args.halfwidth))
fout = join(utils.dumpdir, "crosspk",
"out_{}_{}" + "_{}.p".format(args.halfwidth))
jobs = csiborgtools.fits.split_jobs(n_sims, nproc)[rank]
for n in jobs:
print("Rank {}@{}: saving {}th delta.".format(rank, datetime.now(), n))
# Set the paths
n_sim = ics[n]
paths.set_info(n_sim, paths.get_maximum_snapshot(n_sim))
# Set reader and the box
reader = csiborgtools.read.ParticleReader(paths)
box = csiborgtools.units.BoxUnits(paths)
# Read particles
particles = reader.read_particle(["x", "y", "z", "M"], verbose=False)
# Halfwidth -- particle selection
if args.halfwidth < 0.5:
hw = args.halfwidth
mask = ((0.5 - hw < particles['x']) & (particles['x'] < 0.5 + hw)
& (0.5 - hw < particles['y']) & (particles['y'] < 0.5 + hw)
& (0.5 - hw < particles['z']) & (particles['z'] < 0.5 + hw))
# Subselect the particles
particles = particles[mask]
# Rescale to range [0, 1]
for p in ('x', 'y', 'z'):
particles[p] = (particles[p] - 0.5 + hw) / (2 * hw)
length = box.box2mpc(2 * hw) * box.h
else:
mask = None
length = box.box2mpc(1) * box.h
# Calculate the overdensity field
field = csiborgtools.field.DensityField(particles, length, box, MAS)
delta = field.overdensity_field(args.grid, verbose=False)
aexp = box._aexp
# Try to clean up memory
del field, particles, box, reader, mask
collect()
# Dump the results
with open(ftemp.format(n_sim, "delta") + ".npy", "wb") as f:
numpy.save(f, delta)
joblib.dump([aexp, length], ftemp.format(n_sim, "lengths") + ".p")
# Try to clean up memory
del delta
collect()
comm.Barrier()
# Get off-diagonal elements and append the diagoal
combs = [c for c in combinations(range(n_sims), 2)]
for i in range(n_sims):
combs.append((i, i))
prev_delta = [-1, None, None, None] # i, delta, aexp, length
jobs = csiborgtools.fits.split_jobs(len(combs), nproc)[rank]
for n in jobs:
i, j = combs[n]
print("Rank {}@{}: combination {}.".format(rank, datetime.now(), (i, j)))
# If i same as last time then don't have to load it
if prev_delta[0] == i:
delta_i = prev_delta[1]
aexp_i = prev_delta[2]
length_i = prev_delta[3]
else:
with open(ftemp.format(ics[i], "delta") + ".npy", "rb") as f:
delta_i = numpy.load(f)
aexp_i, length_i = joblib.load(ftemp.format(ics[i], "lengths") + ".p")
# Store in prev_delta
prev_delta[0] = i
prev_delta[1] = delta_i
prev_delta[2] = aexp_i
prev_delta[3] = length_i
# Get jth delta
with open(ftemp.format(ics[j], "delta") + ".npy", "rb") as f:
delta_j = numpy.load(f)
aexp_j, length_j = joblib.load(ftemp.format(ics[j], "lengths") + ".p")
# Verify the difference between the scale factors! Say more than 1%
daexp = abs((aexp_i - aexp_j) / aexp_i)
if daexp > 0.01:
raise ValueError(
"Boxes {} and {} final snapshot scale factors disagree by "
"`{}` percent!".format(ics[i], ics[j], daexp * 100))
# Check how well the boxsizes agree
dlength = abs((length_i - length_j) / length_i)
if dlength > 0.001:
raise ValueError("Boxes {} and {} box sizes disagree by `{}` percent!"
.format(ics[i], ics[j], dlength * 100))
# Calculate the cross power spectrum
Pk = PKL.XPk([delta_i, delta_j], length_i, axis=1, MAS=[MAS, MAS],
threads=1)
joblib.dump(Pk, fout.format(ics[i], ics[j]))
del delta_i, delta_j, Pk
collect()
# Clean up the temp files
comm.Barrier()
if rank == 0:
print("Cleaning up the temporary files...")
for ic in ics:
remove(ftemp.format(ic, "delta") + ".npy")
remove(ftemp.format(ic, "lengths") + ".p")
print("All finished!")