Add redshift space position (#55)

* Add docs

* Delete blank

* Add real to redshift space function

* RSD move back observer

* Convert velocoties to km/s

* Add units to RSP calculation

* Add RSP to catalogues

* Add RSD to angular neighbour search
This commit is contained in:
Richard Stiskalek 2023-05-07 19:07:35 +01:00 committed by GitHub
parent 3df771f1ee
commit 65564849f4
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6 changed files with 2364 additions and 29 deletions

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@ -25,4 +25,4 @@ from .readsim import (MmainReader, ParticleReader, halfwidth_select, # noqa
load_clump_particles, load_parent_particles, read_initcm) load_clump_particles, load_parent_particles, read_initcm)
from .tpcf_summary import TPCFReader # noqa from .tpcf_summary import TPCFReader # noqa
from .utils import (cartesian_to_radec, cols_to_structured, # noqa from .utils import (cartesian_to_radec, cols_to_structured, # noqa
radec_to_cartesian, read_h5) radec_to_cartesian, read_h5, real2redshift)

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@ -27,6 +27,7 @@ CONV_NAME = {
"length": ["x", "y", "z", "peak_x", "peak_y", "peak_z", "Rs", "rmin", "length": ["x", "y", "z", "peak_x", "peak_y", "peak_z", "Rs", "rmin",
"rmax", "r200c", "r500c", "r200m", "x0", "y0", "z0", "rmax", "r200c", "r500c", "r200m", "x0", "y0", "z0",
"lagpatch"], "lagpatch"],
"velocity": ["vx", "vy", "vz"],
"mass": ["mass_cl", "totpartmass", "m200c", "m500c", "mass_mmain", "M", "mass": ["mass_cl", "totpartmass", "m200c", "m500c", "mass_mmain", "M",
"m200m"], "m200m"],
"density": ["rho0"]} "density": ["rho0"]}
@ -93,8 +94,8 @@ class BoxUnits:
@property @property
def H0(self): def H0(self):
r""" r"""
The Hubble parameter at the time of the snapshot The Hubble parameter at the time of the snapshot in units of
in :math:`\mathrm{Mpc} / \mathrm{km} / \mathrm{s}`. :math:`\mathrm{km} \mathrm{s}^{-1} \mathrm{Mpc}^{-1}`.
Returns Returns
------- -------
@ -229,7 +230,7 @@ class BoxUnits:
def box2vel(self, vel): def box2vel(self, vel):
r""" r"""
Convert velocity from box units to :math:`\mathrm{m} / \mathrm{s}^2`. Convert velocity from box units to :math:`\mathrm{km} \mathrm{s}^{-1}`.
Parameters Parameters
---------- ----------
@ -239,9 +240,9 @@ class BoxUnits:
Returns Returns
------- -------
vel : float vel : float
Velocity in :math:`\mathrm{m} / \mathrm{s}^2` Velocity in :math:`\mathrm{km} \mathrm{s}^{-1}`.
""" """
return vel * (1e-2 * self._unit_l / self._unit_t / self._aexp) return vel * (1e-2 * self._unit_l / self._unit_t / self._aexp) * 1e-3
def box2cosmoredshift(self, dist): def box2cosmoredshift(self, dist):
r""" r"""
@ -396,6 +397,7 @@ class BoxUnits:
physical units, such that physical units, such that
- length -> :math:`Mpc`, - length -> :math:`Mpc`,
- mass -> :math:`M_\odot`, - mass -> :math:`M_\odot`,
- velocity -> :math:`\mathrm{km} / \mathrm{s}`,
- density -> :math:`M_\odot / \mathrm{Mpc}^3`. - density -> :math:`M_\odot / \mathrm{Mpc}^3`.
Any other conversions are currently not implemented. Note that the Any other conversions are currently not implemented. Note that the
@ -418,6 +420,7 @@ class BoxUnits:
names = [names] if isinstance(names, str) else names names = [names] if isinstance(names, str) else names
transforms = {"length": self.box2mpc, transforms = {"length": self.box2mpc,
"mass": self.box2solarmass, "mass": self.box2solarmass,
"velocity": self.box2vel,
"density": self.box2dens, "density": self.box2dens,
} }

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@ -22,7 +22,7 @@ from .box_units import BoxUnits
from .paths import CSiBORGPaths from .paths import CSiBORGPaths
from .readsim import ParticleReader from .readsim import ParticleReader
from .utils import (add_columns, cartesian_to_radec, flip_cols, from .utils import (add_columns, cartesian_to_radec, flip_cols,
radec_to_cartesian) radec_to_cartesian, real2redshift)
class BaseCatalogue(ABC): class BaseCatalogue(ABC):
@ -152,6 +152,33 @@ class BaseCatalogue(ABC):
""" """
return numpy.vstack([self["v{}".format(p)] for p in ("x", "y", "z")]).T return numpy.vstack([self["v{}".format(p)] for p in ("x", "y", "z")]).T
def redshift_space_position(self, cartesian=True):
r"""
Redshift space position components. If Cartesian, then in
:math:`\mathrm{cMpc}`. If spherical, then radius is in
:math:`\mathrm{cMpc}`, RA in :math:`[0, 360)` degrees and DEC in
:math:`[-90, 90]` degrees. Note that the position is defined as the
minimum of the gravitationl potential.
Parameters
----------
cartesian : bool, optional
Whether to return the Cartesian or spherical position components.
By default Cartesian.
Returns
-------
pos : 2-dimensional array of shape `(nobjects, 3)`
"""
pos = self.position(cartesian=True)
vel = self.velocity()
origin = [0., 0., 0.]
rsp = real2redshift(pos, vel, origin, self.box, in_box_units=False,
make_copy=False)
if not cartesian:
rsp = cartesian_to_radec(rsp)
return rsp
def angmomentum(self): def angmomentum(self):
""" """
Cartesian angular momentum components of halos in the box coordinate Cartesian angular momentum components of halos in the box coordinate
@ -207,7 +234,7 @@ class BaseCatalogue(ABC):
knn = self.knn(in_initial) knn = self.knn(in_initial)
return knn.radius_neighbors(X, radius, sort_results=True) return knn.radius_neighbors(X, radius, sort_results=True)
def angular_neighbours(self, X, ang_radius, rad_tolerance=None): def angular_neighbours(self, X, ang_radius, in_rsp, rad_tolerance=None):
r""" r"""
Find nearest neighbours within `ang_radius` of query points `X`. Find nearest neighbours within `ang_radius` of query points `X`.
Optionally applies radial tolerance, which is expected to be in Optionally applies radial tolerance, which is expected to be in
@ -219,6 +246,8 @@ class BaseCatalogue(ABC):
Query positions. If 2-dimensional, then RA and DEC in degrees. Query positions. If 2-dimensional, then RA and DEC in degrees.
If 3-dimensional, then radial distance in :math:`\mathrm{cMpc}`, If 3-dimensional, then radial distance in :math:`\mathrm{cMpc}`,
RA and DEC in degrees. RA and DEC in degrees.
in_rsp : bool
Whether to use redshift space positions of haloes.
ang_radius : float ang_radius : float
Angular radius in degrees. Angular radius in degrees.
rad_tolerance : float, optional rad_tolerance : float, optional
@ -234,6 +263,9 @@ class BaseCatalogue(ABC):
assert X.ndim == 2 assert X.ndim == 2
# We first get positions of haloes in this catalogue, store their # We first get positions of haloes in this catalogue, store their
# radial distance and normalise them to unit vectors. # radial distance and normalise them to unit vectors.
if in_rsp:
pos = self.redshift_space_position(cartesian=True)
else:
pos = self.position(in_initial=False, cartesian=True) pos = self.position(in_initial=False, cartesian=True)
raddist = numpy.linalg.norm(pos, axis=1) raddist = numpy.linalg.norm(pos, axis=1)
pos /= raddist.reshape(-1, 1) pos /= raddist.reshape(-1, 1)
@ -329,7 +361,8 @@ class ClumpsCatalogue(BaseCatalogue):
for p in ("x", "y", "z"): for p in ("x", "y", "z"):
self._data[p] -= 0.5 self._data[p] -= 0.5
names = ["x", "y", "z", "mass_cl", "totpartmass", "rho0", "r200c", names = ["x", "y", "z", "mass_cl", "totpartmass", "rho0", "r200c",
"r500c", "m200c", "m500c", "r200m", "m200m"] "r500c", "m200c", "m500c", "r200m", "m200m",
"vx", "vy", "vz"]
self._data = self.box.convert_from_boxunits(self._data, names) self._data = self.box.convert_from_boxunits(self._data, names)
if maxdist is not None: if maxdist is not None:
dist = numpy.sqrt(self._data["x"]**2 + self._data["y"]**2 dist = numpy.sqrt(self._data["x"]**2 + self._data["y"]**2
@ -420,7 +453,8 @@ class HaloCatalogue(BaseCatalogue):
for p in ("x", "y", "z"): for p in ("x", "y", "z"):
self._data[p] -= 0.5 self._data[p] -= 0.5
names = ["x", "y", "z", "M", "totpartmass", "rho0", "r200c", names = ["x", "y", "z", "M", "totpartmass", "rho0", "r200c",
"r500c", "m200c", "m500c", "r200m", "m200m"] "r500c", "m200c", "m500c", "r200m", "m200m",
"vx", "vy", "vz"]
self._data = self.box.convert_from_boxunits(self._data, names) self._data = self.box.convert_from_boxunits(self._data, names)
if load_initial: if load_initial:

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@ -21,7 +21,6 @@ from os.path import isfile
import numpy import numpy
from tqdm import tqdm from tqdm import tqdm
############################################################################### ###############################################################################
# Overlap of two simulations # # Overlap of two simulations #
############################################################################### ###############################################################################
@ -602,6 +601,11 @@ class NPairsOverlap:
return len(self.pairs) return len(self.pairs)
###############################################################################
# Various support functions. #
###############################################################################
def binned_resample_mean(x, y, prob, bins, nresample=50, seed=42): def binned_resample_mean(x, y, prob, bins, nresample=50, seed=42):
""" """
Calculate binned average of `y` by MC resampling. Each point is kept with Calculate binned average of `y` by MC resampling. Each point is kept with

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@ -80,6 +80,51 @@ def radec_to_cartesian(X, isdeg=True):
return dist * numpy.vstack([x, y, z]).T return dist * numpy.vstack([x, y, z]).T
def real2redshift(pos, vel, origin, box, in_box_units, make_copy=True):
r"""
Convert real-space position to redshift space position.
Parameters
----------
pos : 2-dimensional array `(nsamples, 3)`
Real-space Cartesian position components.
vel : 2-dimensional array `(nsamples, 3)`
Cartesian velocity components.
origin : 1-dimensional array `(3,)`
Origin of the coordinate system in the `pos` reference frame.
box : py:class:`csiborg.read.BoxUnits`
Box units.
in_box_units: bool
Whether `pos` and `vel` are in box units. If not, position is assumed
to be in :math:`\mathrm{Mpc}`, velocity in
:math:`\mathrm{km} \mathrm{s}^{-1}` and math:`h=0.705`, or otherwise
matching the box.
make_copy : bool, optional
Whether to make a copy of `pos` before modifying it.
Returns
-------
pos : 2-dimensional array `(nsamples, 3)`
Redshift-space Cartesian position components, with an observer assumed
at the `origin`.
"""
a = box._aexp
H0 = box.box_H0 if in_box_units else box.H0
if make_copy:
pos = numpy.copy(pos)
for i in range(3):
pos[:, i] -= origin[i]
norm2 = numpy.sum(pos**2, axis=1)
dot = numpy.einsum("ij,ij->i", pos, vel)
pos *= (1 + a / H0 * dot / norm2).reshape(-1, 1)
for i in range(3):
pos[:, i] += origin[i]
return pos
############################################################################### ###############################################################################
# Array manipulation # # Array manipulation #
############################################################################### ###############################################################################

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