mirror of
https://github.com/Richard-Sti/csiborgtools.git
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Density field calculation (#58)
* Add iterative density field generation * Edit particle halfwidth selection * Update import * Remove old file * Add position wrapping * Add RSD support * Add density field calculation * Edit paths to the density field * Flip argument order * Edit documentation * Edit docs * update nb
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parent
4265315b47
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8 changed files with 227 additions and 241 deletions
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@ -16,16 +16,14 @@
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Density field and cross-correlation calculations.
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Density field and cross-correlation calculations.
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"""
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"""
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from abc import ABC
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from abc import ABC
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from warnings import warn
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import MAS_library as MASL
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import MAS_library as MASL
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import numpy
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import numpy
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import Pk_library as PKL
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import smoothing_library as SL
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import smoothing_library as SL
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from tqdm import trange
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from tqdm import trange
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from .utils import force_single_precision
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from .utils import force_single_precision
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from ..read.utils import radec_to_cartesian
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from ..read.utils import radec_to_cartesian, real2redshift
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class BaseField(ABC):
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class BaseField(ABC):
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@ -189,11 +187,6 @@ class DensityField(BaseField):
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Parameters
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Parameters
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----------
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----------
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pos : 2-dimensional array of shape `(N, 3)`
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Particle position array. Columns must be ordered as `['x', 'y', 'z']`.
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The positions are assumed to be in box units, i.e. :math:`\in [0, 1 ]`.
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mass : 1-dimensional array of shape `(N,)`
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Particle mass array. Assumed to be in box units.
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box : :py:class:`csiborgtools.read.BoxUnits`
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box : :py:class:`csiborgtools.read.BoxUnits`
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The simulation box information and transformations.
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The simulation box information and transformations.
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MAS : str
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MAS : str
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@ -205,52 +198,11 @@ class DensityField(BaseField):
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----------
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----------
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[1] https://pylians3.readthedocs.io/
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[1] https://pylians3.readthedocs.io/
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"""
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"""
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_pos = None
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_mass = None
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def __init__(self, pos, mass, box, MAS):
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def __init__(self, box, MAS):
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self.pos = pos
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self.mass = mass
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self.box = box
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self.box = box
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self.MAS = MAS
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self.MAS = MAS
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@property
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def pos(self):
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"""
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Particle position array.
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Returns
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-------
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particles : 2-dimensional array
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"""
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return self._particles
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@pos.setter
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def pos(self, pos):
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assert pos.ndim == 2
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warn("Flipping the `x` and `z` coordinates of the particle positions.",
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UserWarning, stacklevel=1)
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pos[:, [0, 2]] = pos[:, [2, 0]]
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pos = force_single_precision(pos, "particle_position")
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self._pos = pos
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@property
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def mass(self):
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"""
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Particle mass array.
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Returns
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-------
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mass : 1-dimensional array
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"""
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return self._mass
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@mass.setter
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def mass(self, mass):
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assert mass.ndim == 1
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mass = force_single_precision(mass, "particle_mass")
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self._mass = mass
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def smoothen(self, field, smooth_scale, threads=1):
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def smoothen(self, field, smooth_scale, threads=1):
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"""
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"""
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Smooth a field with a Gaussian filter.
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Smooth a field with a Gaussian filter.
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@ -294,17 +246,28 @@ class DensityField(BaseField):
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delta -= 1
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delta -= 1
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return delta
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return delta
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def __call__(self, grid, smooth_scale=None, verbose=True):
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def __call__(self, parts, grid, in_rsp, flip_xz=True, nbatch=30,
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verbose=True):
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"""
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"""
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Calculate the density field using a Pylians routine [1, 2].
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Calculate the density field using a Pylians routine [1, 2].
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Iteratively loads the particles into memory, flips their `x` and `z`
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coordinates. Particles are assumed to be in box units, with positions
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in [0, 1] and observer in the centre of the box if RSP is applied.
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Parameters
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Parameters
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----------
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----------
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parts : 2-dimensional array of shape `(n_parts, 7)`
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Particle positions, velocities and masses.
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Columns are: `x`, `y`, `z`, `vx`, `vy`, `vz`, `M`.
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grid : int
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grid : int
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Grid size.
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Grid size.
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smooth_scale : float, optional
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in_rsp : bool
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Gaussian kernal scale to smoothen the density field, in box units.
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Whether to calculate the density field in redshift space.
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verbose : bool
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flip_xz : bool, optional
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Whether to flip the `x` and `z` coordinates.
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nbatch : int, optional
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Number of batches to split the particle loading into.
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verbose : bool, optional
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Verbosity flag.
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Verbosity flag.
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Returns
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Returns
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@ -318,12 +281,32 @@ class DensityField(BaseField):
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[2] https://github.com/franciscovillaescusa/Pylians3/blob/master
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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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/library/MAS_library/MAS_library.pyx
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"""
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"""
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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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rho = numpy.zeros((grid, grid, grid), dtype=numpy.float32)
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MASL.MA(self.pos, rho, self.boxsize, self.MAS, W=self.mass,
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verbose=verbose)
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nparts = parts.shape[0]
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if smooth_scale is not None:
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batch_size = nparts // nbatch
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rho = self.smoothen(rho, smooth_scale)
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start = 0
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for __ in trange(nbatch + 1) if verbose else range(nbatch + 1):
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end = min(start + batch_size, nparts)
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pos = parts[start:end]
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pos, vel, mass = pos[:, :3], pos[:, 3:6], pos[:, 6]
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pos = force_single_precision(pos, "particle_position")
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vel = force_single_precision(vel, "particle_velocity")
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mass = force_single_precision(mass, "particle_mass")
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if flip_xz:
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pos[:, [0, 2]] = pos[:, [2, 0]]
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vel[:, [0, 2]] = vel[:, [2, 0]]
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if in_rsp:
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pos = real2redshift(pos, vel, [0.5, 0.5, 0.5], self.box,
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in_box_units=True, periodic_wrap=True,
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make_copy=False)
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MASL.MA(pos, rho, self.boxsize, self.MAS, W=mass, verbose=False)
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if end == nparts:
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break
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start = end
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return rho
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return rho
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@ -21,7 +21,7 @@ from .overlap_summary import (NPairsOverlap, PairOverlap, # noqa
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binned_resample_mean)
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binned_resample_mean)
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from .paths import CSiBORGPaths # noqa
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from .paths import CSiBORGPaths # noqa
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from .pk_summary import PKReader # noqa
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from .pk_summary import PKReader # noqa
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from .readsim import (MmainReader, ParticleReader, halfwidth_select, # noqa
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from .readsim import (MmainReader, ParticleReader, halfwidth_mask, # noqa
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load_clump_particles, load_parent_particles, read_initcm)
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load_clump_particles, load_parent_particles, read_initcm)
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from .tpcf_summary import TPCFReader # noqa
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from .tpcf_summary import TPCFReader # noqa
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from .utils import (cartesian_to_radec, cols_to_structured, # noqa
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from .utils import (cartesian_to_radec, cols_to_structured, # noqa
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@ -329,16 +329,18 @@ class CSiBORGPaths:
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fname = f"parts_{str(nsim).zfill(5)}.h5"
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fname = f"parts_{str(nsim).zfill(5)}.h5"
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return join(fdir, fname)
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return join(fdir, fname)
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def density_field_path(self, mas, nsim):
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def density_field_path(self, MAS, nsim, in_rsp):
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"""
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"""
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Path to the files containing the calculated density fields.
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Path to the files containing the calculated density fields.
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Parameters
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Parameters
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----------
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----------
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mas : str
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MAS : str
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Mass-assignment scheme. Currently only SPH is supported.
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Mass-assignment scheme. Currently only SPH is supported.
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nsim : int
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nsim : int
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IC realisation index.
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IC realisation index.
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in_rsp : bool
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Whether the density field is calculated in redshift space.
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Returns
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Returns
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-------
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-------
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@ -348,7 +350,9 @@ class CSiBORGPaths:
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if not isdir(fdir):
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if not isdir(fdir):
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makedirs(fdir)
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makedirs(fdir)
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warn(f"Created directory `{fdir}`.", UserWarning, stacklevel=1)
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warn(f"Created directory `{fdir}`.", UserWarning, stacklevel=1)
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fname = f"density_{mas}_{str(nsim).zfill(5)}.npy"
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fname = f"density_{MAS}_{str(nsim).zfill(5)}.npy"
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if in_rsp:
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fname = fname.replace("density", "density_rsp")
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return join(fdir, fname)
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return join(fdir, fname)
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def knnauto_path(self, run, nsim=None):
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def knnauto_path(self, run, nsim=None):
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@ -534,34 +534,23 @@ def read_initcm(nsim, srcdir, fname="clump_{}_cm.npy"):
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return None
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return None
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def halfwidth_select(hw, particles):
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def halfwidth_mask(pos, hw):
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"""
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"""
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Select particles that in a cube of size `2 hw`, centered at the origin.
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Mask of particles in a region of width `2 hw, centered at the origin.
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Note that this directly modifies the original array and throws away
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particles outside the central region.
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Parameters
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Parameters
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----------
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----------
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pos : 2-dimensional array of shape `(nparticles, 3)`
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Particle positions, in box units.
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hw : float
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hw : float
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Central region halfwidth.
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Central region half-width.
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particles : structured array
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Particle array with keys `x`, `y`, `z`.
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Returns
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Returns
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-------
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-------
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particles : structured array
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mask : 1-dimensional boolean array of shape `(nparticles, )`
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The modified particle array.
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"""
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"""
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assert 0 < hw < 0.5
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assert 0 < hw < 0.5
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mask = ((0.5 - hw < particles['x']) & (particles['x'] < 0.5 + hw)
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return numpy.all((0.5 - hw < pos) & (pos < 0.5 + hw), axis=1)
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& (0.5 - hw < particles['y']) & (particles['y'] < 0.5 + hw)
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& (0.5 - hw < particles['z']) & (particles['z'] < 0.5 + hw))
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# Subselect the particles
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particles = particles[mask]
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# Rescale to range [0, 1]
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for p in ('x', 'y', 'z'):
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particles[p] = (particles[p] - 0.5 + hw) / (2 * hw)
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return particles
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def load_clump_particles(clid, particles, clump_map, clid2map):
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def load_clump_particles(clid, particles, clump_map, clid2map):
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return dist * numpy.vstack([x, y, z]).T
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return dist * numpy.vstack([x, y, z]).T
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def real2redshift(pos, vel, origin, box, in_box_units, make_copy=True):
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def real2redshift(pos, vel, origin, box, in_box_units, periodic_wrap=True,
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make_copy=True):
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r"""
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r"""
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Convert real-space position to redshift space position.
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Convert real-space position to redshift space position.
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to be in :math:`\mathrm{Mpc}`, velocity in
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to be in :math:`\mathrm{Mpc}`, velocity in
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:math:`\mathrm{km} \mathrm{s}^{-1}` and math:`h=0.705`, or otherwise
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:math:`\mathrm{km} \mathrm{s}^{-1}` and math:`h=0.705`, or otherwise
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matching the box.
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matching the box.
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periodic_wrap : bool, optional
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Whether to wrap around the box, particles may be outside the default
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bounds once RSD is applied.
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make_copy : bool, optional
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make_copy : bool, optional
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Whether to make a copy of `pos` before modifying it.
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Whether to make a copy of `pos` before modifying it.
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for i in range(3):
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for i in range(3):
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pos[:, i] += origin[i]
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pos[:, i] += origin[i]
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if periodic_wrap:
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boxsize = 1. if in_box_units else box.box2mpc(1.)
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# Wrap around the box: x > 1 -> x - 1, x < 0 -> x + 1
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pos[pos > boxsize] -= boxsize
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pos[pos < 0] += boxsize
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return pos
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return pos
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File diff suppressed because one or more lines are too long
69
scripts/field_density.py
Normal file
69
scripts/field_density.py
Normal file
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@ -0,0 +1,69 @@
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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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"""
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MPI script to calculate the density fields on CSiBORG simulations in the final
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snapshot.
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"""
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from argparse import ArgumentParser
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from datetime import datetime
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from distutils.util import strtobool
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import numpy
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from mpi4py import MPI
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try:
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import csiborgtools
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except ModuleNotFoundError:
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import sys
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sys.path.append("../")
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import csiborgtools
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comm = MPI.COMM_WORLD
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rank = comm.Get_rank()
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nproc = comm.Get_size()
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verbose = nproc == 1
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parser = ArgumentParser()
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parser.add_argument("--ics", type=int, nargs="+", default=None,
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help="IC realisations. If `-1` processes all simulations.")
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parser.add_argument("--grid", type=int, help="Grid resolution.")
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parser.add_argument("--in_rsp", type=lambda x: bool(strtobool(x)),
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help="Calculate the density field in redshift space?")
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parser.add_argument("--MAS", type=str, choices=["NGP", "CIC", "TSC", "PCS"])
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args = parser.parse_args()
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paths = csiborgtools.read.CSiBORGPaths(**csiborgtools.paths_glamdring)
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if args.ics is None or args.ics[0] == -1:
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ics = paths.get_ics(tonew=False)
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else:
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ics = args.ics
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for i in csiborgtools.fits.split_jobs(len(ics), nproc)[rank]:
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nsim = ics[i]
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print(f"{datetime.now()}: rank {rank} working on simulation {nsim}.",
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flush=True)
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nsnap = max(paths.get_snapshots(nsim))
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box = csiborgtools.read.BoxUnits(nsnap, nsim, paths)
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parts = csiborgtools.read.read_h5(paths.particles_path(nsim))["particles"]
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density_generator = csiborgtools.field.DensityField(box, args.MAS)
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rho = density_generator(parts, args.grid, in_rsp=args.in_rsp,
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verbose=verbose)
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fout = paths.density_field_path(args.MAS, nsim, args.in_rsp)
|
||||||
|
print(f"{datetime.now()}: rank {rank} saving output to `{fout}`.")
|
||||||
|
numpy.save(fout, rho)
|
|
@ -1,127 +0,0 @@
|
||||||
# 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 evaluate field properties at the galaxy positions.
|
|
||||||
"""
|
|
||||||
from argparse import ArgumentParser
|
|
||||||
from datetime import datetime
|
|
||||||
from os import remove
|
|
||||||
from os.path import join
|
|
||||||
|
|
||||||
import numpy
|
|
||||||
from mpi4py import MPI
|
|
||||||
|
|
||||||
try:
|
|
||||||
import csiborgtools
|
|
||||||
except ModuleNotFoundError:
|
|
||||||
import sys
|
|
||||||
sys.path.append("../")
|
|
||||||
import csiborgtools
|
|
||||||
|
|
||||||
import utils
|
|
||||||
|
|
||||||
dumpdir = "/mnt/extraspace/rstiskalek/csiborg/"
|
|
||||||
parser = ArgumentParser()
|
|
||||||
parser.add_argument("--survey", type=str, choices=["SDSS"])
|
|
||||||
parser.add_argument("--grid", type=int)
|
|
||||||
parser.add_argument("--MAS", type=str, choices=["NGP", "CIC", "TSC", "PCS"])
|
|
||||||
parser.add_argument("--halfwidth", type=float)
|
|
||||||
parser.add_argument("--smooth_scale", type=float, default=None)
|
|
||||||
args = parser.parse_args()
|
|
||||||
# Smooth scale of 0 means no smoothing. Note that this is in Mpc/h
|
|
||||||
args.smooth_scale = None if args.smooth_scale == 0 else args.smooth_scale
|
|
||||||
|
|
||||||
# Get MPI things
|
|
||||||
comm = MPI.COMM_WORLD
|
|
||||||
rank = comm.Get_rank()
|
|
||||||
nproc = comm.Get_size()
|
|
||||||
|
|
||||||
# Galaxy positions
|
|
||||||
survey = utils.surveys[args.survey]()()
|
|
||||||
pos = numpy.vstack([survey[p] for p in ("DIST", "RA", "DEC")]).T
|
|
||||||
pos = pos.astype(numpy.float32)
|
|
||||||
|
|
||||||
# File paths
|
|
||||||
fname = "out_{}_{}_{}_{}_{}".format(
|
|
||||||
survey.name, args.grid, args.MAS, args.halfwidth, args.smooth_scale)
|
|
||||||
ftemp = join(dumpdir, "temp_fields", fname + "_{}.npy")
|
|
||||||
fperm = join(dumpdir, "fields", fname + ".npy")
|
|
||||||
|
|
||||||
# Edit depending on what is calculated
|
|
||||||
dtype = {"names": ["delta", "phi"], "formats": [numpy.float32] * 2}
|
|
||||||
|
|
||||||
# CSiBORG simulation paths
|
|
||||||
paths = csiborgtools.read.CSiBORGPaths(**csiborgtools.paths_glamdring)
|
|
||||||
ics = paths.get_ics(tonew=False)
|
|
||||||
nsims = len(ics)
|
|
||||||
|
|
||||||
for n in csiborgtools.utils.split_jobs(nsims, nproc)[rank]:
|
|
||||||
print("Rank {}@{}: working on {}th IC.".format(rank, datetime.now(), n),
|
|
||||||
flush=True)
|
|
||||||
nsim = ics[n]
|
|
||||||
nsnap = max(paths.get_snapshots(nsim))
|
|
||||||
reader = csiborgtools.read.ParticleReader(paths)
|
|
||||||
box = csiborgtools.read.BoxUnits(nsnap, nsim, paths)
|
|
||||||
|
|
||||||
# Read particles and select a subset of them
|
|
||||||
particles = reader.read_particle(nsnap, nsim, ["x", "y", "z", "M"],
|
|
||||||
verbose=False)
|
|
||||||
if args.halfwidth < 0.5:
|
|
||||||
particles = csiborgtools.read.halfwidth_select(
|
|
||||||
args.halfwidth, particles)
|
|
||||||
length = box.box2mpc(2 * args.halfwidth) * box.h # Mpc/h
|
|
||||||
else:
|
|
||||||
length = box.box2mpc(1) * box.h # Mpc/h
|
|
||||||
|
|
||||||
# Initialise the field object and output array
|
|
||||||
field = csiborgtools.field.DensityField(particles, length, box, args.MAS)
|
|
||||||
out = numpy.full(pos.shape[0], numpy.nan, dtype=dtype)
|
|
||||||
|
|
||||||
# Calculate the overdensity field and interpolate at galaxy positions
|
|
||||||
feval = field.overdensity_field(args.grid, args.smooth_scale,
|
|
||||||
verbose=False)
|
|
||||||
out["delta"] = field.evaluate_sky(feval, pos=pos, isdeg=True)[0]
|
|
||||||
|
|
||||||
# Potential
|
|
||||||
feval = field.potential_field(args.grid, args.smooth_scale, verbose=False)
|
|
||||||
out["phi"] = field.evaluate_sky(feval, pos=pos, isdeg=True)[0]
|
|
||||||
|
|
||||||
# Calculate the remaining fields
|
|
||||||
# ...
|
|
||||||
# ...
|
|
||||||
|
|
||||||
# Dump the results
|
|
||||||
with open(ftemp.format(nsim), "wb") as f:
|
|
||||||
numpy.save(f, out)
|
|
||||||
|
|
||||||
# Wait for all ranks to finish
|
|
||||||
comm.Barrier()
|
|
||||||
if rank == 0:
|
|
||||||
print("Collecting files...", flush=True)
|
|
||||||
|
|
||||||
out = numpy.full((nsims, pos.shape[0]), numpy.nan, dtype=dtype)
|
|
||||||
|
|
||||||
for n in range(nsims):
|
|
||||||
nsim = ics[n]
|
|
||||||
with open(ftemp.format(nsim), "rb") as f:
|
|
||||||
fin = numpy.load(f, allow_pickle=True)
|
|
||||||
for name in dtype["names"]:
|
|
||||||
out[name][n, ...] = fin[name]
|
|
||||||
# Remove the temporary file
|
|
||||||
remove(ftemp.format(nsim))
|
|
||||||
|
|
||||||
print("Saving results to `{}`.".format(fperm), flush=True)
|
|
||||||
with open(fperm, "wb") as f:
|
|
||||||
numpy.save(f, out)
|
|
Loading…
Reference in a new issue