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Potential (#13)
* add basic density field * Add TODO * add field smoothing * update how pos are calculated * add transforms both ways * add import * add sky density * add make skymap func * update TODO * update gitignore * add potential field calculation * delete boxsize setter * add tidal tensor
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7 changed files with 379 additions and 27 deletions
1
.gitignore
vendored
1
.gitignore
vendored
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@ -16,3 +16,4 @@ build/*
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csiborgtools.egg-info/*
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csiborgtools.egg-info/*
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scripts/playground_*
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scripts/playground_*
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scripts/playground.ipynb
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scripts/playground.ipynb
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Pylians3/*
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@ -13,4 +13,4 @@
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# with this program; if not, write to the Free Software Foundation, Inc.,
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# with this program; if not, write to the Free Software Foundation, Inc.,
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# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
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# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
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from csiborgtools import (read, match, utils, units, fits) # noqa
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from csiborgtools import (read, match, utils, units, fits, field) # noqa
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16
csiborgtools/field/__init__.py
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16
csiborgtools/field/__init__.py
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@ -0,0 +1,16 @@
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# Copyright (C) 2022 Richard Stiskalek
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# This program is free software; you can redistribute it and/or modify it
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# under the terms of the GNU General Public License as published by the
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# Free Software Foundation; either version 3 of the License, or (at your
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# option) any later version.
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#
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# This program is distributed in the hope that it will be useful, but
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# WITHOUT ANY WARRANTY; without even the implied warranty of
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# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General
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# Public License for more details.
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#
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# You should have received a copy of the GNU General Public License along
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# with this program; if not, write to the Free Software Foundation, Inc.,
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# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
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from .density import DensityField # noqa
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323
csiborgtools/field/density.py
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323
csiborgtools/field/density.py
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@ -0,0 +1,323 @@
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# Copyright (C) 2022 Richard Stiskalek
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# This program is free software; you can redistribute it and/or modify it
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# under the terms of the GNU General Public License as published by the
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# Free Software Foundation; either version 3 of the License, or (at your
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# option) any later version.
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#
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# This program is distributed in the hope that it will be useful, but
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# WITHOUT ANY WARRANTY; without even the implied warranty of
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# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General
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# Public License for more details.
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#
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# You should have received a copy of the GNU General Public License along
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# with this program; if not, write to the Free Software Foundation, Inc.,
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# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
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import numpy
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import MAS_library as MASL
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import smoothing_library as SL
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from warnings import warn
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from tqdm import trange
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from ..units import (BoxUnits, radec_to_cartesian)
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class DensityField:
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"""
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Density field calculations. Based primarily on routines of Pylians [1].
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Parameters
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----------
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particles : structured array
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Particle array. Must contain keys `['x', 'y', 'z', 'M']`.
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box : :py:class:`csiborgtools.units.BoxUnits`
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The simulation box information and transformations.
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References
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----------
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[1] https://pylians3.readthedocs.io/
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"""
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_particles = None
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_boxsize = None
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_box = None
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def __init__(self, particles, box):
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self.particles = particles
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self.box = box
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self._boxsize = 1.
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@property
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def particles(self):
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"""
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Particles structured array.
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Returns
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-------
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particles : structured array
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"""
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return self._particles
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@particles.setter
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def particles(self, particles):
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"""Set `particles`, checking it has the right columns."""
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if any(p not in particles.dtype.names for p in ('x', 'y', 'z', 'M')):
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raise ValueError("`particles` must be a structured array "
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"containing `['x', 'y', 'z', 'M']`.")
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self._particles = particles
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@property
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def box(self):
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"""
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The simulation box information and transformations.
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Returns
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-------
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box : :py:class:`csiborgtools.units.BoxUnits`
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"""
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return self._box
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@box.setter
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def box(self, box):
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"""Set the simulation box."""
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if not isinstance(box, BoxUnits):
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raise TypeError("`box` must be `BoxUnits` instance.")
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self._box = box
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@property
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def boxsize(self):
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"""
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Boxsize.
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Returns
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-------
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boxsize : float
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"""
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return self._boxsize
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@staticmethod
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def _force_f32(x, name):
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if x.dtype != numpy.float32:
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warn("Converting `{}` to float32.".format(name))
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x = x.astype(numpy.float32)
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return x
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def density_field(self, grid, verbose=True):
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"""
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Calculate the density field using a Pylians routine [1, 2]. Enforces
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float32 precision.
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Parameters
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----------
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grid : int
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The grid size.
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verbose : float, optional
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A verbosity flag. By default `True`.
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Returns
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-------
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rho : 3-dimensional array of shape `(grid, grid, grid)`.
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Density field.
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References
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----------
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[1] https://pylians3.readthedocs.io/
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[2] https://github.com/franciscovillaescusa/Pylians3/blob/master
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/library/MAS_library/MAS_library.pyx
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"""
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pos = numpy.vstack([self.particles[p] for p in ('x', 'y', 'z')]).T
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pos *= self.boxsize
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pos = self._force_f32(pos, "pos")
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weights = self._force_f32(self.particles['M'], 'M')
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MAS = "CIC" # Cloud in cell
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# Pre-allocate and do calculations
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rho = numpy.zeros((grid, grid, grid), dtype=numpy.float32)
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MASL.MA(pos, rho, self.boxsize, MAS, W=weights, verbose=verbose)
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return rho
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def overdensity_field(self, grid, verbose=True):
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r"""
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Calculate the overdensity field using Pylians routines.
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Defined as :math:`\rho/ <\rho> - 1`.
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Parameters
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----------
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grid : int
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The grid size.
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verbose : float, optional
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A verbosity flag. By default `True`.
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Returns
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-------
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overdensity : 3-dimensional array of shape `(grid, grid, grid)`.
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Overdensity field.
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"""
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# Get the overdensity
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delta = self.density_field(grid, verbose)
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delta /= delta.mean()
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delta -= 1
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return delta
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def potential_field(self, grid, verbose=True):
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"""
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Calculate the potential field using Pylians routines.
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Parameters
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----------
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grid : int
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The grid size.
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verbose : float, optional
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A verbosity flag. By default `True`.
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Returns
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-------
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potential : 3-dimensional array of shape `(grid, grid, grid)`.
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Potential field.
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"""
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delta = self.overdensity_field(grid, verbose)
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if verbose:
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print("Calculating potential from the overdensity..")
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return MASL.potential(delta, self.box._omega_m, self.box._aexp, "CIC")
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def tensor_field(self, grid, verbose=True):
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"""
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Calculate the tidal tensor field.
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Parameters
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----------
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grid : int
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The grid size.
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verbose : float, optional
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A verbosity flag. By default `True`.
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Returns
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-------
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tidal_tensor : :py:class:`MAS_library.tidal_tensor`
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Tidal tensor object, whose attributes `tidal_tensor.Tij` contain
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the relevant tensor components.
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"""
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delta = self.overdensity_field(grid, verbose)
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return MASL.tidal_tensor(delta, self.box._omega_m, self.box._aexp,
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"CIC")
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def smooth_field(self, field, scale, threads=1):
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"""
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Smooth a field with a Gaussian filter.
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Parameters
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----------
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field : 3-dimensional array of shape `(grid, grid, grid)`
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The field to be smoothed.
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scale : float
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The smoothing scale of the Gaussian filter. Units must match that
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of `self.boxsize`.
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threads : int, optional
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Number of threads. By default 1.
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Returns
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-------
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smoothed_field : 3-dimensional array of shape `(grid, grid, grid)`
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"""
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Filter = "Gaussian"
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grid = field.shape[0]
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# FFT of the filter
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W_k = SL.FT_filter(self.boxsize, scale, grid, Filter, threads)
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return SL.field_smoothing(field, W_k, threads)
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def evaluate_field(self, pos, field):
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"""
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Evaluate the field at Cartesian coordinates.
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Parameters
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----------
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pos : 2-dimensional array of shape `(n_samples, 3)`
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Positions to evaluate the density field. The coordinates span range
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of [0, boxsize].
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field : 3-dimensional array of shape `(grid, grid, grid)`
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The density field that is to be interpolated.
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Returns
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-------
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interp_field : 1-dimensional array of shape `(n_samples,).
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Interpolated field at `pos`.
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"""
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self._force_f32(pos, "pos")
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density_interpolated = numpy.zeros(pos.shape[0], dtype=numpy.float32)
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MASL.CIC_interp(field, self.boxsize, pos, density_interpolated)
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return density_interpolated
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def evaluate_sky(self, pos, field, isdeg=True):
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"""
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Evaluate the field at given distance, right ascension and declination.
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Assumes that the observed is in the centre of the box.
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Parameters
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----------
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pos : 2-dimensional array of shape `(n_samples, 3)`
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Spherical coordinates to evaluate the field. Should be distance,
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right ascension, declination, respectively.
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field : 3-dimensional array of shape `(grid, grid, grid)`
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The density field that is to be interpolated. Assumed to be defined
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on a Cartesian grid.
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isdeg : bool, optional
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Whether `ra` and `dec` are in degres. By default `True`.
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Returns
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-------
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interp_field : 1-dimensional array of shape `(n_samples,).
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Interpolated field at `pos`.
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"""
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self._force_f32(pos, "pos")
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X = numpy.vstack(
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radec_to_cartesian(*(pos[:, i] for i in range(3)), isdeg)).T
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X = X.astype(numpy.float32)
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# Place the observer at the center of the box
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X += 0.5 * self.boxsize
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return self.evaluate_field(X, field)
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def make_sky_map(self, ra, dec, field, dist_marg, isdeg=True,
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verbose=True):
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"""
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Make a sky map of a density field. Places the observed in the center of
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the box and evaluates the field in directions `ra`, `dec`. At each such
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position evaluates the field at distances `dist_marg` and sums these
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interpolated values of the field.
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Parameters
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----------
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ra, dec : 1-dimensional arrays of shape `(n_pos, )`
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Directions to evaluate the field. Assumes `dec` is in [-90, 90]
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degrees (or equivalently in radians).
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field : 3-dimensional array of shape `(grid, grid, grid)`
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The density field that is to be interpolated. Assumed to be defined
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on a Cartesian grid `[0, self.boxsize]^3`.
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dist_marg : 1-dimensional array
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Radial distances to evaluate the field.
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isdeg : bool, optional
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Whether `ra` and `dec` are in degres. By default `True`.
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verbose : bool, optional
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Verbosity flag. By default `True`.
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Returns
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-------
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interp_field : 1-dimensional array of shape `(n_pos, )`.
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"""
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# Angular positions at which to evaluate the field
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Nang = ra.size
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pos = numpy.vstack([ra, dec]).T
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# Now loop over the angular positions, each time evaluating a vector
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# of distances. Pre-allocate arrays for speed
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ra_loop = numpy.ones_like(dist_marg)
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dec_loop = numpy.ones_like(dist_marg)
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pos_loop = numpy.ones((dist_marg.size, 3), dtype=numpy.float32)
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out = numpy.zeros(Nang, dtype=numpy.float32)
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for i in trange(Nang) if verbose else range(Nang):
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# Get the position vector for this choice of theta, phi
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ra_loop[:] = pos[i, 0]
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dec_loop[:] = pos[i, 1]
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pos_loop[:] = numpy.vstack([dist_marg, ra_loop, dec_loop]).T
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# Evaluate and sum it up
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out[i] = numpy.sum(self.evaluate_sky(pos_loop, field, isdeg))
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return out
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@ -163,7 +163,9 @@ class HaloCatalogue:
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data = data[data["m500"] > min_m500]
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data = data[data["m500"] > min_m500]
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# Now calculate spherical coordinates
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# Now calculate spherical coordinates
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d, ra, dec = cartesian_to_radec(data)
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d, ra, dec = cartesian_to_radec(
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data["peak_x"], data["peak_y"], data["peak_z"])
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data = add_columns(data, [d, ra, dec], ["dist", "ra", "dec"])
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data = add_columns(data, [d, ra, dec], ["dist", "ra", "dec"])
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# Cut on separation
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# Cut on separation
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@ -13,5 +13,5 @@
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# with this program; if not, write to the Free Software Foundation, Inc.,
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# with this program; if not, write to the Free Software Foundation, Inc.,
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||||||
# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
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# 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
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||||||
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from .transforms import cartesian_to_radec # noqa
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from .transforms import cartesian_to_radec, radec_to_cartesian # noqa
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from .box_units import (BoxUnits) # noqa
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from .box_units import (BoxUnits) # noqa
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@ -19,39 +19,49 @@ Various coordinate transformations.
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import numpy
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import numpy
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def cartesian_to_radec(arr, xpar="peak_x", ypar="peak_y", zpar="peak_z"):
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def cartesian_to_radec(x, y, z):
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r"""
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"""
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||||||
Extract `x`, `y`, and `z` coordinates from a record array `arr` and
|
Calculate the radial distance, right ascension in [0, 360) degrees and
|
||||||
calculate the radial distance :math:`r` in coordinate units, right
|
declination [-90, 90] degrees. Note, the observer should be placed in the
|
||||||
ascension :math:`\mathrm{RA} \in [0, 360)` degrees and declination
|
middle of the box.
|
||||||
:math:`\delta \in [-90, 90]` degrees.
|
|
||||||
|
|
||||||
Parameters
|
Parameters
|
||||||
----------
|
----------
|
||||||
arr : record array
|
x, y, z : 1-dimensional arrays
|
||||||
Record array with the Cartesian coordinates.
|
Cartesian coordinates.
|
||||||
xpar : str, optional
|
|
||||||
Name of the x coordinate in the record array.
|
|
||||||
ypar : str, optional
|
|
||||||
Name of the y coordinate in the record array.
|
|
||||||
zpar : str, optional
|
|
||||||
Name of the z coordinate in the record array.
|
|
||||||
|
|
||||||
Returns
|
Returns
|
||||||
-------
|
-------
|
||||||
dist : 1-dimensional array
|
dist, ra, dec : 1-dimensional arrays
|
||||||
Radial distance.
|
Radial distance, right ascension and declination.
|
||||||
ra : 1-dimensional array
|
|
||||||
Right ascension.
|
|
||||||
dec : 1-dimensional array
|
|
||||||
Declination.
|
|
||||||
"""
|
"""
|
||||||
x, y, z = arr[xpar], arr[ypar], arr[zpar]
|
|
||||||
|
|
||||||
dist = numpy.sqrt(x**2 + y**2 + z**2)
|
dist = numpy.sqrt(x**2 + y**2 + z**2)
|
||||||
dec = numpy.rad2deg(numpy.arcsin(z/dist))
|
dec = numpy.rad2deg(numpy.arcsin(z/dist))
|
||||||
ra = numpy.rad2deg(numpy.arctan2(y, x))
|
ra = numpy.rad2deg(numpy.arctan2(y, x))
|
||||||
# Make sure RA in the correct range
|
# Make sure RA in the correct range
|
||||||
ra[ra < 0] += 360
|
ra[ra < 0] += 360
|
||||||
|
|
||||||
return dist, ra, dec
|
return dist, ra, dec
|
||||||
|
|
||||||
|
|
||||||
|
def radec_to_cartesian(dist, ra, dec, isdeg=True):
|
||||||
|
"""
|
||||||
|
Convert distance, right ascension and declination to Cartesian coordinates.
|
||||||
|
|
||||||
|
Parameters
|
||||||
|
----------
|
||||||
|
dist, ra, dec : 1-dimensional arrays
|
||||||
|
The spherical coordinates.
|
||||||
|
isdeg : bool, optional
|
||||||
|
Whether `ra` and `dec` are in degres. By default `True`.
|
||||||
|
|
||||||
|
Returns
|
||||||
|
-------
|
||||||
|
x, y, z : 1-dimensional arrays
|
||||||
|
Cartesian coordinates.
|
||||||
|
"""
|
||||||
|
if isdeg:
|
||||||
|
ra = numpy.deg2rad(ra)
|
||||||
|
dec = numpy.deg2rad(dec)
|
||||||
|
x = dist * numpy.cos(dec) * numpy.cos(ra)
|
||||||
|
y = dist * numpy.cos(dec) * numpy.sin(ra)
|
||||||
|
z = dist * numpy.sin(dec)
|
||||||
|
return x, y, z
|
||||||
|
|
Loading…
Reference in a new issue