background

• distances (2015) Output cosmological distance measures for dynamical dark energy

cmb_lensing

• kappa_beam (1.0) Apply smoothing function to cross-correlations with CMB kappa in harmonic space.

• kappa_ell_cut (1.0) Apply minimum and maximum ell to cross-power spectra with CMB kappa.

luminosity_function

• Joachimi_Bridle_alpha (1.0) Calculate the gradient of the galaxy luminosity function at the limiting magnitude of the survey.

likelihood

• planck (1.0) Likelihood function of CMB from Planck

• mgs_bao (1409.3242) Compute the likelihood against SDSS MGS data

• Cluster_mass (1.0) Likelihood of z=1.59 Cluster mass from Santos et al. 2011

• BOSS (1303.4486) Compute the likelihood of supplied fsigma8(z=0.57), H(z=0.57), D_a(z=0.57), omegamh2, bsigma8(z=0.57)

• pantheon (2018) Likelihood of the Pantheon supernova analysis

• planck_sz (1.0) Prior on sigma_8 * Omega_M ** 0.3 from Planck SZ cluster counts

• wmap_shift (1.0) Massively simplified WMAP9 likelihood reduced to just shift parameter

• BICEP2 (20140314) Compute the likelihood of the supplied CMB power spectra

• wmap (5) Likelihood function of CMB from WMAP

• wmap (4.1) Likelihood function of CMB from WMAP

• shear_xi (1.0) Compute the likelihood of a tomographic shear correlation function data set

• Riess16 (2016) Likelihood of hubble parameter H0 from Riess et al 2.4% supernova sample

• Riess11 (2011) Likelihood of hubble parameter H0 from Riess et al supernova sample

• Extreme_Value_Statistics (1.0) PDF of the maximum cluster mass given cosmological parameters

• 6dFGS () Compute the likelihood of supplied D_v or fsigma8(z=0.067)

• BBN (PDG13) Simple prior on Omega_b h^2 from light element abundances

• fgas (2014) Likelihood of galaxy cluster gas-mass fractions

• WiggleZBao (1401.0358v2) Compute the likelihood of the supplied expansion history against WiggleZ BAO data

• 2pt (1) Generic 2-point measurement Gaussian likelihood

• boss_dr12 (1607.03155v1) Compute the likelihood of the supplied expansion and growth history against BOSS DR12 data

• JulloLikelihood (2012) Likelihood of Jullo et al (2012) measurements of a galaxy bias sample

• planck2015_simple (2) Simplified Likelihood function of CMB from Planck 2015 TT TE EE data

• planck2015 (2) Likelihood function of CMB from Planck 2015 data

planck2015_simple

• planck2015_lowl (1) Planck 2015 commander likelihood made suitable for Fisher foreacasts

mass_function

• Press_Schechter_MF (1) Code to compute the PressSchechter mass function given Pk from CAMB, based on Komatsu's CRL

• Sheth-Tormen MF (1) Code to compute the Sheth-Tormen mass function given Pk from CAMB, based on Komatsu's CRL

• Tinker_MF (1) Code to compute the Tinker et al. mass function given Pk from CAMB, based on Komatsu's CRL

boltzmann

• isitgr-camb (1.1) Modified version of CAMB to implement phenomenological modified gravity models

• extrapolate (1.0) Simple log-linear extrapolation of P(k) to high k

• mgcamb (Feb14) Modified Gravity Boltzmann and background integrator for BG, CMB, and matter power

• sigma_r (1.0) Compute anisotropy dispersion sigma(R,z)

• sigma_cpp (1.0) Compute anisotropy dispersion sigma(R,z) in cpp

• camb (Jan15) Boltzmann and background integrator for BG, CMB, and matter power

• camb (Nov13) Boltzmann and background integrator for BG, CMB, and matter power (Note some settings in this module may not be consistent with other modules e.g. the Planck likelihood. Camb 2015 is recommended in this case)

• class (2.4.1) Boltzmann and background integrator for BG, CMB, matter power, and more

• Halofit_Takahashi (Camb-Nov-13) Compute non-linear matter power spectrum

• Halofit (Camb-Oct-09) Compute non-linear matter power spectrum

number_density

• load_nz (1) Load a number density n(z) for weak lensing from a file

• gaussian_window (1) Compute Gaussian n(z) window functions for weak lensing bins

• load_nz_fits (1) Load a number density n(z) from a FITS file

• photoz_bias (1) Modify a set of loaded n(z) distributions with a multiplicative or additive bias

• smail (1) Compute window functions for photometric n(z)

shear

• apply_astrophysical_biases (1.0) Apply various astrophysical biases to the matter power spectrum P(k,z)

• cl_to_xi_nicaea (1.0) Compute WL correlation functions xi+, xi- from C_ell

• wl_spectra (1.0) Compute various weak lensing C_ell from P(k,z) with the Limber integral

• cl_to_corr (1.0) Compute correlation functions xi+, xi-, w, and gamma_t from C_ell

• wl_spectra_ppf (1.0) Compute weak lensing C_ell from P(k,z) and MG D(k,z) with the Limber integral

• shear_bias (1) Modify a set of calculated shear C_ell with a multiplicative bias

• add_intrinsic (1.0) Sum together intrinsic aligments with shear signal

bias

• constant_bias (1) Apply a galaxy bias constant with k and z.

• clerkin (1) Compute galaxy bias as function of k, z for 3-parameter Clerkin et al 2014 model

• no_bias (1) Generate galaxy power P(k) as though galaxies were unbiased DM tracers

structure

• growth_factor (1) returns linear growth factor and growth rate for flat cosmology with either const w or variable DE eos w(a) = w + (1-a)*wa

• FrankenEmu (2.0) Emulate N-body simulations to compute nonlinear matter power

• mead (Camb-Feb-2018) Uses an extended Halo model to compute non-linear and baryonic power

• extract_growth (1) returns growth factor and growth rate by examining large-scale P(k)

• mead (1.0) Uses an extended Halo model to compute non-linear and baryonic power

• CosmicEmu (2.0) Emulate N-body simulations to compute nonlinear matter power

• CRL_Eisenstein_Hu (1) Komatsu's CRL code to compute the power spectrum using EH fitting formula.

• project_2d (1.0) Project 3D power spectra to 2D tomographic bins using the Limber approximation

strong_lensing

• strong_lens_time_delays (1)

• balmes (1)

supernovae

• jla (3) Supernova likelihood for SDSS-II/SNLS3

• jla (6) Supernova likelihood for SDSS-II/SNLS3

intrinsic_alignments

• linear_alignments (1.0) Compute the terms P_II and P_GI which go into intrinsic aligment calculations

• ia_z_powerlap (2.0)

utility

• sigma8_rescale (1.0) Rescale structure measures to use a specified sigma_8

• stop (1.0) Enters python debugger.

• consistent_parameters (1.0) Deduce missing cosmological parameters and check consistency

• BBN-Consistency (0705.0290) Compute consistent Helium fraction from baryon density given BBN