pyRSD
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Getting Started
Install pyRSD
Overview
Quickstart
RSD
Specifying the Cosmology
Interfacing with CLASS
Halo Zel’dovich Perturbation Theory
Galaxy Power Spectrum
Quasar Power Spectrum
RSDFit
Getting Started
Specifying the Data
Specifying the Theory
Running the Fits
Exploring the Results
Advanced Patterns
pyRSD
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A
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B
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C
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D
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E
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F
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G
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H
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I
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J
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K
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L
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N
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O
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P
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R
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T
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U
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W
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Z
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__call__() (pyRSD.pygcl.CorrelationFunction method)
(pyRSD.pygcl.LinearPS method)
(pyRSD.pygcl.ZeldovichCF method)
(pyRSD.pygcl.ZeldovichP00 method)
(pyRSD.pygcl.ZeldovichP01 method)
(pyRSD.pygcl.ZeldovichP11 method)
(pyRSD.rsd.hzpt.HaloZeldovichCF00 method)
(pyRSD.rsd.hzpt.HaloZeldovichCFhm method)
(pyRSD.rsd.hzpt.HaloZeldovichP00 method)
(pyRSD.rsd.hzpt.HaloZeldovichP01 method)
(pyRSD.rsd.hzpt.HaloZeldovichP11 method)
(pyRSD.rsd.hzpt.HaloZeldovichPhm method)
__init__() (pyRSD.pygcl.CorrelationFunction method)
(pyRSD.pygcl.LinearPS method)
(pyRSD.pygcl.ZeldovichCF method)
(pyRSD.pygcl.ZeldovichP00 method)
(pyRSD.pygcl.ZeldovichP01 method)
(pyRSD.pygcl.ZeldovichP11 method)
(pyRSD.rsd.hzpt.HaloZeldovichCF00 method)
(pyRSD.rsd.hzpt.HaloZeldovichCFhm method)
(pyRSD.rsd.hzpt.HaloZeldovichP00 method)
(pyRSD.rsd.hzpt.HaloZeldovichP01 method)
(pyRSD.rsd.hzpt.HaloZeldovichP11 method)
(pyRSD.rsd.hzpt.HaloZeldovichPhm method)
(pyRSD.rsdfit.analysis.driver.AnalysisDriver method)
A
A_s() (pyRSD.pygcl.Cosmology method)
add() (pyRSD.rsdfit.parameters.ParameterSet method)
add_many() (pyRSD.rsdfit.parameters.ParameterSet method)
AnalysisDriver (class in pyRSD.rsdfit.analysis.driver)
analytic (pyRSD.rsdfit.parameters.Parameter attribute)
as_dict() (pyRSD.rsdfit.results.EmceeResults method)
B
bounded (pyRSD.rsdfit.parameters.Parameter attribute)
broadband() (pyRSD.rsd.hzpt.HaloZeldovichCF00 method)
(pyRSD.rsd.hzpt.HaloZeldovichCFhm method)
(pyRSD.rsd.hzpt.HaloZeldovichP00 method)
(pyRSD.rsd.hzpt.HaloZeldovichP01 method)
(pyRSD.rsd.hzpt.HaloZeldovichP11 method)
(pyRSD.rsd.hzpt.HaloZeldovichPhm method)
burnin (pyRSD.rsdfit.results.EmceeParameter attribute)
(pyRSD.rsdfit.results.EmceeResults attribute)
C
chains() (pyRSD.rsdfit.results.EmceeResults method)
check() (pyRSD.rsdfit.theory.GalaxyPowerTheory method)
chi2() (pyRSD.rsdfit.FittingDriver method)
clear() (pyRSD.rsdfit.parameters.ParameterSet method)
clone() (pyRSD.rsd.cosmology.Cosmology method)
constrained (pyRSD.rsdfit.parameters.Parameter attribute)
(pyRSD.rsdfit.parameters.ParameterSet attribute)
constrained_dtype (pyRSD.rsdfit.parameters.ParameterSet attribute)
constrained_names (pyRSD.rsdfit.parameters.ParameterSet attribute)
constrained_values (pyRSD.rsdfit.parameters.ParameterSet attribute)
constrained_values() (pyRSD.rsdfit.results.EmceeResults method)
constraint_derivative() (pyRSD.rsdfit.parameters.ParameterSet method)
copy() (pyRSD.rsdfit.parameters.ParameterSet method)
(pyRSD.rsdfit.results.EmceeResults method)
(pyRSD.rsdfit.results.LBFGSResults method)
corr() (pyRSD.rsdfit.results.EmceeResults method)
CorrelationFunction (class in pyRSD.pygcl)
Cosmology (class in pyRSD.pygcl)
(class in pyRSD.rsd.cosmology)
covariance (pyRSD.rsdfit.data.PowerData attribute)
covariance_Nmocks (pyRSD.rsdfit.data.PowerData attribute)
covariance_rescaling (pyRSD.rsdfit.data.PowerData attribute)
cutsky_gaussian_covariance() (pyRSD.rsdfit.data.PoleCovarianceMatrix class method)
D
D_z() (in module pyRSD.pygcl)
Da_z() (in module pyRSD.pygcl)
data_file (pyRSD.rsdfit.data.PowerData attribute)
Dc_z() (in module pyRSD.pygcl)
default_params() (pyRSD.rsd.GalaxySpectrum method)
delayed_asteval() (pyRSD.rsdfit.parameters.ParameterSet method)
description (pyRSD.rsdfit.parameters.Parameter attribute)
dlnprior (pyRSD.rsdfit.parameters.Parameter attribute)
(pyRSD.rsdfit.theory.GalaxyPowerTheory attribute)
Dm_z() (in module pyRSD.pygcl)
dof (pyRSD.rsdfit.FittingDriver attribute)
dtype (pyRSD.rsdfit.parameters.Parameter attribute)
dump() (pyRSD.rsdfit.parameters.ParameterSet method)
dumps() (pyRSD.rsdfit.parameters.ParameterSet method)
dV() (in module pyRSD.pygcl)
E
ells (pyRSD.rsdfit.data.PowerData attribute)
EmceeParameter (class in pyRSD.rsdfit.results)
EmceeResults (class in pyRSD.rsdfit.results)
error_rescaling (pyRSD.rsdfit.results.EmceeParameter attribute)
(pyRSD.rsdfit.results.EmceeResults attribute)
evaluate_grad_lnlike() (pyRSD.rsdfit.theory.GalaxyPowerTheory method)
EvaluateTransfer() (pyRSD.pygcl.Cosmology method)
expr (pyRSD.rsdfit.parameters.Parameter attribute)
F
f_z() (in module pyRSD.pygcl)
fiducial (pyRSD.rsdfit.parameters.Parameter attribute)
(pyRSD.rsdfit.results.EmceeParameter attribute)
fisher() (pyRSD.rsdfit.FittingDriver method)
fitting_range (pyRSD.rsdfit.data.PowerData attribute)
FittingDriver (class in pyRSD.rsdfit)
flat_trace (pyRSD.rsdfit.results.EmceeParameter attribute)
free (pyRSD.rsdfit.parameters.ParameterSet attribute)
free_dtype (pyRSD.rsdfit.parameters.ParameterSet attribute)
free_fiducial (pyRSD.rsdfit.theory.GalaxyPowerTheory attribute)
free_names (pyRSD.rsdfit.parameters.ParameterSet attribute)
free_values (pyRSD.rsdfit.parameters.ParameterSet attribute)
from_array() (pyRSD.rsdfit.data.PowerMeasurements class method)
from_astropy() (pyRSD.rsd.cosmology.Cosmology class method)
from_directory() (pyRSD.rsdfit.FittingDriver class method)
from_file() (pyRSD.rsdfit.parameters.ParameterSet class method)
from_npz() (pyRSD.rsdfit.results.EmceeResults class method)
(pyRSD.rsdfit.results.LBFGSResults class method)
from_plaintext() (pyRSD.rsdfit.data.PkmuCovarianceMatrix class method)
(pyRSD.rsdfit.data.PoleCovarianceMatrix class method)
(pyRSD.rsdfit.data.PowerMeasurements class method)
fromkeys() (pyRSD.rsdfit.parameters.ParameterSet method)
G
GalaxyPowerTheory (class in pyRSD.rsdfit.theory)
GalaxySpectrum (class in pyRSD.rsd)
get() (pyRSD.rsdfit.parameters.ParameterSet method)
get_kmu_pairs() (pyRSD.rsdfit.theory.GalaxyPowerTheory method)
get_value_from_prior() (pyRSD.rsdfit.parameters.Parameter method)
grad_minus_lnlike() (pyRSD.rsdfit.FittingDriver method)
grid_file (pyRSD.rsdfit.data.PowerData attribute)
H
h() (pyRSD.pygcl.Cosmology method)
H0() (pyRSD.pygcl.Cosmology method)
H_z() (in module pyRSD.pygcl)
HaloZeldovichCF00 (class in pyRSD.rsd.hzpt)
HaloZeldovichCFhm (class in pyRSD.rsd.hzpt)
HaloZeldovichP00 (class in pyRSD.rsd.hzpt)
HaloZeldovichP01 (class in pyRSD.rsd.hzpt)
HaloZeldovichP11 (class in pyRSD.rsd.hzpt)
HaloZeldovichPhm (class in pyRSD.rsd.hzpt)
has_fiducial (pyRSD.rsdfit.parameters.Parameter attribute)
has_prior (pyRSD.rsdfit.parameters.Parameter attribute)
help() (pyRSD.rsdfit.data.PowerData static method)
I
inverse_scale() (pyRSD.rsdfit.theory.GalaxyPowerTheory method)
items() (pyRSD.rsdfit.parameters.ParameterSet method)
iterations (pyRSD.rsdfit.results.EmceeResults attribute)
(pyRSD.rsdfit.results.LBFGSResults attribute)
J
jointplot_2d() (pyRSD.rsdfit.results.EmceeResults method)
K
k_max() (pyRSD.pygcl.Cosmology method)
k_min() (pyRSD.pygcl.Cosmology method)
k_pivot() (pyRSD.pygcl.Cosmology method)
kdeplot_2d() (pyRSD.rsdfit.results.EmceeResults method)
keys() (pyRSD.rsdfit.parameters.ParameterSet method)
L
LBFGSResults (class in pyRSD.rsdfit.results)
LinearPS (class in pyRSD.pygcl)
ln_1e10_A_s() (pyRSD.pygcl.Cosmology method)
lnlike() (pyRSD.rsdfit.FittingDriver method)
lnprior (pyRSD.rsdfit.parameters.Parameter attribute)
(pyRSD.rsdfit.theory.GalaxyPowerTheory attribute)
lnprior_constrained (pyRSD.rsdfit.theory.GalaxyPowerTheory attribute)
lnprior_free (pyRSD.rsdfit.theory.GalaxyPowerTheory attribute)
lnprob() (pyRSD.rsdfit.FittingDriver method)
load() (pyRSD.rsdfit.parameters.ParameterSet method)
loads() (pyRSD.rsdfit.parameters.ParameterSet method)
loc (pyRSD.rsdfit.parameters.Parameter attribute)
locs (pyRSD.rsdfit.parameters.ParameterSet attribute)
lower (pyRSD.rsdfit.parameters.Parameter attribute)
M
marginalized_errors() (pyRSD.rsdfit.FittingDriver method)
max (pyRSD.rsdfit.parameters.Parameter attribute)
max_bound (pyRSD.rsdfit.parameters.Parameter attribute)
max_ellprime (pyRSD.rsdfit.data.PowerData attribute)
max_lnprob (pyRSD.rsdfit.results.EmceeResults attribute)
max_lnprob_constrained_values() (pyRSD.rsdfit.results.EmceeResults method)
max_lnprob_values() (pyRSD.rsdfit.results.EmceeResults method)
mean (pyRSD.rsdfit.results.EmceeParameter attribute)
median (pyRSD.rsdfit.results.EmceeParameter attribute)
min (pyRSD.rsdfit.parameters.Parameter attribute)
min_bound (pyRSD.rsdfit.parameters.Parameter attribute)
minus_lnlike() (pyRSD.rsdfit.FittingDriver method)
mode (pyRSD.rsdfit.data.PowerData attribute)
model (pyRSD.rsdfit.FittingDriver attribute)
model_callable() (pyRSD.rsdfit.theory.GalaxyPowerTheory method)
move_to_end() (pyRSD.rsdfit.parameters.ParameterSet method)
mu (pyRSD.rsdfit.parameters.Parameter attribute)
mu_bounds (pyRSD.rsdfit.data.PowerData attribute)
N
n_s() (pyRSD.pygcl.Cosmology method)
Nb (pyRSD.rsdfit.FittingDriver attribute)
ndim (pyRSD.rsdfit.results.EmceeResults attribute)
(pyRSD.rsdfit.results.LBFGSResults attribute)
(pyRSD.rsdfit.theory.GalaxyPowerTheory attribute)
Np (pyRSD.rsdfit.FittingDriver attribute)
O
Omega0_b() (pyRSD.pygcl.Cosmology method)
Omega0_cdm() (pyRSD.pygcl.Cosmology method)
Omega0_fld() (pyRSD.pygcl.Cosmology method)
Omega0_g() (pyRSD.pygcl.Cosmology method)
Omega0_k() (pyRSD.pygcl.Cosmology method)
Omega0_lambda() (pyRSD.pygcl.Cosmology method)
Omega0_m() (pyRSD.pygcl.Cosmology method)
Omega0_r() (pyRSD.pygcl.Cosmology method)
Omega0_ur() (pyRSD.pygcl.Cosmology method)
Omega_m_z() (in module pyRSD.pygcl)
one_sigma (pyRSD.rsdfit.results.EmceeParameter attribute)
output_value (pyRSD.rsdfit.parameters.Parameter attribute)
P
Parameter (class in pyRSD.rsdfit.parameters)
ParameterSet (class in pyRSD.rsdfit.parameters)
peak (pyRSD.rsdfit.results.EmceeParameter attribute)
peak_constrained_values() (pyRSD.rsdfit.results.EmceeResults method)
peak_values() (pyRSD.rsdfit.results.EmceeResults method)
periodic_gaussian_covariance() (pyRSD.rsdfit.data.PkmuCovarianceMatrix class method)
(pyRSD.rsdfit.data.PoleCovarianceMatrix class method)
pkmu_gradient (pyRSD.rsdfit.theory.GalaxyPowerTheory attribute)
PkmuCovarianceMatrix (class in pyRSD.rsdfit.data)
Planck13 (pyRSD.rsd.cosmology attribute)
Planck15 (pyRSD.rsd.cosmology attribute)
plot() (pyRSD.rsdfit.FittingDriver method)
plot_correlation() (pyRSD.rsdfit.results.EmceeResults method)
plot_residuals() (pyRSD.rsdfit.FittingDriver method)
plot_timeline() (pyRSD.rsdfit.results.EmceeResults method)
plot_triangle() (pyRSD.rsdfit.results.EmceeResults method)
PoleCovarianceMatrix (class in pyRSD.rsdfit.data)
poles() (pyRSD.rsd.GalaxySpectrum method)
pop() (pyRSD.rsdfit.parameters.ParameterSet method)
popitem() (pyRSD.rsdfit.parameters.ParameterSet method)
power() (pyRSD.rsd.GalaxySpectrum method)
PowerData (class in pyRSD.rsdfit.data)
PowerMeasurements (class in pyRSD.rsdfit.data)
prepare_params() (pyRSD.rsdfit.parameters.ParameterSet method)
preserve() (pyRSD.rsdfit.theory.GalaxyPowerTheory method)
pretty_print() (pyRSD.rsdfit.parameters.ParameterSet method)
pretty_repr() (pyRSD.rsdfit.parameters.ParameterSet method)
prior (pyRSD.rsdfit.parameters.Parameter attribute)
prior_name (pyRSD.rsdfit.parameters.Parameter attribute)
R
reduced_chi2() (pyRSD.rsdfit.FittingDriver method)
register_function() (pyRSD.rsdfit.parameters.ParameterSet method)
results (pyRSD.rsdfit.FittingDriver attribute)
rho_bar_z() (in module pyRSD.pygcl)
rho_crit() (pyRSD.pygcl.Cosmology method)
rho_crit_z() (in module pyRSD.pygcl)
rs_drag() (pyRSD.pygcl.Cosmology method)
run() (pyRSD.rsdfit.FittingDriver method)
S
scale (pyRSD.rsdfit.parameters.Parameter attribute)
scale() (pyRSD.rsdfit.theory.GalaxyPowerTheory method)
scale_gradient() (pyRSD.rsdfit.parameters.Parameter method)
(pyRSD.rsdfit.theory.GalaxyPowerTheory method)
scales (pyRSD.rsdfit.parameters.ParameterSet attribute)
set() (pyRSD.rsdfit.parameters.Parameter method)
set_expr_eval() (pyRSD.rsdfit.parameters.Parameter method)
set_fit_results() (pyRSD.rsdfit.FittingDriver method)
set_free_parameters() (pyRSD.rsdfit.theory.GalaxyPowerTheory method)
setdefault() (pyRSD.rsdfit.parameters.ParameterSet method)
SetSigma8AtZ() (pyRSD.pygcl.LinearPS method)
(pyRSD.pygcl.ZeldovichCF method)
(pyRSD.pygcl.ZeldovichP00 method)
(pyRSD.pygcl.ZeldovichP01 method)
(pyRSD.pygcl.ZeldovichP11 method)
setup_bounds() (pyRSD.rsdfit.parameters.Parameter method)
sigma (pyRSD.rsdfit.parameters.Parameter attribute)
sigma8() (pyRSD.pygcl.Cosmology method)
Sigma8_z() (in module pyRSD.pygcl)
sorted_1d_corrs() (pyRSD.rsdfit.results.EmceeResults method)
statistics (pyRSD.rsdfit.data.PowerData attribute)
stderr (pyRSD.rsdfit.results.EmceeParameter attribute)
summarize_fit() (pyRSD.rsdfit.results.EmceeResults method)
(pyRSD.rsdfit.results.LBFGSResults method)
T
tau_reio() (pyRSD.pygcl.Cosmology method)
Tcmb() (pyRSD.pygcl.Cosmology method)
three_sigma (pyRSD.rsdfit.results.EmceeParameter attribute)
to_class() (pyRSD.rsd.cosmology.Cosmology method)
to_dict() (pyRSD.rsdfit.parameters.Parameter method)
(pyRSD.rsdfit.parameters.ParameterSet method)
to_file() (pyRSD.rsdfit.data.PowerData method)
(pyRSD.rsdfit.parameters.ParameterSet method)
(pyRSD.rsdfit.theory.GalaxyPowerTheory method)
to_npz() (pyRSD.rsdfit.results.EmceeResults method)
(pyRSD.rsdfit.results.LBFGSResults method)
to_plaintext() (pyRSD.rsdfit.data.PkmuCovarianceMatrix method)
(pyRSD.rsdfit.data.PoleCovarianceMatrix method)
(pyRSD.rsdfit.data.PowerMeasurements method)
trace() (pyRSD.rsdfit.results.EmceeParameter method)
two_sigma (pyRSD.rsdfit.results.EmceeParameter attribute)
U
update() (pyRSD.rsdfit.parameters.Parameter method)
(pyRSD.rsdfit.parameters.ParameterSet method)
update_constraints() (pyRSD.rsdfit.parameters.ParameterSet method)
update_fiducial() (pyRSD.rsdfit.parameters.ParameterSet method)
update_param() (pyRSD.rsdfit.parameters.ParameterSet method)
update_values() (pyRSD.rsdfit.parameters.ParameterSet method)
upper (pyRSD.rsdfit.parameters.Parameter attribute)
usedata (pyRSD.rsdfit.data.PowerData attribute)
V
V() (in module pyRSD.pygcl)
value (pyRSD.rsdfit.parameters.Parameter attribute)
values() (pyRSD.rsdfit.parameters.ParameterSet method)
(pyRSD.rsdfit.results.EmceeResults method)
valuesdict() (pyRSD.rsdfit.parameters.ParameterSet method)
verify_param_ordering() (pyRSD.rsdfit.results.EmceeResults method)
(pyRSD.rsdfit.results.LBFGSResults method)
W
w0_fld() (pyRSD.pygcl.Cosmology method)
wa_fld() (pyRSD.pygcl.Cosmology method)
walkers (pyRSD.rsdfit.results.EmceeResults attribute)
window_file (pyRSD.rsdfit.data.PowerData attribute)
within_bounds() (pyRSD.rsdfit.parameters.Parameter method)
WMAP5 (pyRSD.rsd.cosmology attribute)
WMAP7 (pyRSD.rsd.cosmology attribute)
WMAP9 (pyRSD.rsd.cosmology attribute)
Z
z_drag() (pyRSD.pygcl.Cosmology method)
z_reio() (pyRSD.pygcl.Cosmology method)
zeldovich() (pyRSD.rsd.hzpt.HaloZeldovichCF00 method)
(pyRSD.rsd.hzpt.HaloZeldovichCFhm method)
(pyRSD.rsd.hzpt.HaloZeldovichP00 method)
(pyRSD.rsd.hzpt.HaloZeldovichP01 method)
(pyRSD.rsd.hzpt.HaloZeldovichP11 method)
(pyRSD.rsd.hzpt.HaloZeldovichPhm method)
ZeldovichCF (class in pyRSD.pygcl)
ZeldovichP00 (class in pyRSD.pygcl)
ZeldovichP01 (class in pyRSD.pygcl)
ZeldovichP11 (class in pyRSD.pygcl)
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