s_mu_tpcf¶

halotools.mock_observables.
s_mu_tpcf
(sample1, s_bins, mu_bins, sample2=None, randoms=None, period=None, do_auto=True, do_cross=True, estimator=u'Natural', num_threads=1, approx_cell1_size=None, approx_cell2_size=None, approx_cellran_size=None, seed=None)[source] [edit on github]¶ Calculate the redshift space correlation function, \(\xi(s, \mu)\)
Divide redshift space into bins of radial separation and angle to to the lineofsight (LOS). This is a prestep for calculating correlation function multipoles.
The first two dimensions (x, y) define the plane for perpendicular distances. The third dimension (z) is used for parallel distances. i.e. x,y positions are on the plane of the sky, and z is the radial distance coordinate. This is the ‘distant observer’ approximation.
Example calls to this function appear in the documentation below. See the Formatting your xyz coordinates for Mock Observables calculations documentation page for instructions on how to transform your coordinate position arrays into the format accepted by the
sample1
andsample2
arguments.Parameters: sample1 : array_like
Npts1 x 3 numpy array containing 3D positions of points. See the Formatting your xyz coordinates for Mock Observables calculations documentation page, or the Examples section below, for instructions on how to transform your coordinate position arrays into the format accepted by the
sample1
andsample2
arguments. Length units are comoving and assumed to be in Mpc/h, here and throughout Halotools.s_bins : array_like
numpy array of shape (num_s_bin_edges, ) storing the \(s\) boundaries defining the bins in which pairs are counted.
mu_bins : array_like
numpy array of shape (num_mu_bin_edges, ) storing the \(\cos(\theta_{\rm LOS})\) boundaries defining the bins in which pairs are counted. All values must be between [0,1].
sample2 : array_like, optional
Npts2 x 3 array containing 3D positions of points. Passing
sample2
as an input permits the calculation of the crosscorrelation function. Default is None, in which case only the autocorrelation function will be calculated.randoms : array_like, optional
Nran x 3 array containing 3D positions of randomly distributed points. If no randoms are provided (the default option), calculation of the tpcf can proceed using analytical randoms (only valid for periodic boundary conditions).
period : array_like, optional
Length3 sequence defining the periodic boundary conditions in each dimension. If you instead provide a single scalar, Lbox, period is assumed to be the same in all Cartesian directions. If set to None (the default option), PBCs are set to infinity, in which case
randoms
must be provided. Length units are comoving and assumed to be in Mpc/h, here and throughout Halotools.do_auto : boolean, optional
Boolean determines whether the autocorrelation function will be calculated and returned. Default is True.
do_cross : boolean, optional
Boolean determines whether the crosscorrelation function will be calculated and returned. Only relevant when
sample2
is also provided. Default is True for the case wheresample2
is provided, otherwise False.estimator : string, optional
Statistical estimator for the tpcf. Options are ‘Natural’, ‘DavisPeebles’, ‘Hewett’ , ‘Hamilton’, ‘LandySzalay’ Default is
Natural
.num_threads : int, optional
Number of threads to use in calculation, where parallelization is performed using the python
multiprocessing
module. Default is 1 for a purely serial calculation, in which case a multiprocessing Pool object will never be instantiated. A string ‘max’ may be used to indicate that the pair counters should use all available cores on the machine.approx_cell1_size : array_like, optional
Length3 array serving as a guess for the optimal manner by how points will be apportioned into subvolumes of the simulation box. The optimum choice unavoidably depends on the specs of your machine. Default choice is to use Lbox/10 in each dimension, which will return reasonable result performance for most usecases. Performance can vary sensitively with this parameter, so it is highly recommended that you experiment with this parameter when carrying out performancecritical calculations.
approx_cell2_size : array_like, optional
Analogous to
approx_cell1_size
, but for sample2. See comments forapprox_cell1_size
for details.approx_cellran_size : array_like, optional
Analogous to
approx_cell1_size
, but for randoms. See comments forapprox_cell1_size
for details.seed : int, optional
Random number seed used to randomly downsample data, if applicable. Default is None, in which case downsampling will be stochastic.
Returns: correlation_function(s) : np.ndarray
Numpy array of shape (num_s_bin_edges1, num_mu_bin_edges1) containing the correlation function \(\xi(s, \mu)\) computed in each of the bins defined by input
s_bins
andmu_bins
.\[1 + \xi(s,\mu) = \mathrm{DD}(s,\mu) / \mathrm{RR}(s,\mu)\]if
estimator
is set to ‘Natural’, where \(\mathrm{DD}(s,\mu)\) is calculated by the pair counter, and \(\mathrm{RR}(s,\mu)\) is counted internally using “analytic randoms” ifrandoms
is set to None (see notes for further details).If
sample2
is not None (and not exactly the same assample1
), three arrays of shape len(s_bins)1 by len(mu_bins)1 are returned:\[\xi_{11}(s,\mu), \xi_{12}(s,\mu), \xi_{22}(s,\mu),\]the autocorrelation of
sample1
, the crosscorrelation betweensample1
andsample2
, and the autocorrelation ofsample2
, respectively. Ifdo_auto
ordo_cross
is set to False, the appropriate result(s) are returned.Notes
Let \(\vec{s}\) be the radial vector connnecting two points. The magnitude, \(s\), is:
\[s = \sqrt{r_{\parallel}^2+r_{\perp}^2},\]where \(r_{\parallel}\) is the separation parallel to the LOS and \(r_{\perp}\) is the separation perpednicular to the LOS. \(\mu\) is the cosine of the angle, \(\theta_{\rm LOS}\), between the LOS and \(\vec{s}\):
\[\mu = \cos(\theta_{\rm LOS}) \equiv r_{\parallel}/s.\]Pairs are counted using
npairs_s_mu
.If the
period
argument is passed in, the ith coordinate of all points must be between 0 and period[i].Examples
For demonstration purposes we create a randomly distributed set of points within a periodic cube with Lbox = 250 Mpc/h
>>> Npts = 1000 >>> Lbox = 250.
>>> x = np.random.uniform(0, Lbox, Npts) >>> y = np.random.uniform(0, Lbox, Npts) >>> z = np.random.uniform(0, Lbox, Npts)
We transform our x, y, z points into the array shape used by the paircounter by taking the transpose of the result of
numpy.vstack
. This boilerplate transformation is used throughout themock_observables
subpackage:>>> sample1 = np.vstack((x,y,z)).T
Alternatively, you may use the
return_xyz_formatted_array
convenience function for this same purpose, which provides additional wrapper behavior aroundnumpy.vstack
such as placing points into redshiftspace.>>> s_bins = np.logspace(1, 1, 10) >>> mu_bins = np.linspace(0, 1, 50) >>> xi = s_mu_tpcf(sample1, s_bins, mu_bins, period=Lbox)