1.3.5

• angular_diameter_distance2 fix and allow for vector arguments
• Support vector arguments for physical_time, physical_time_a1_a2 and conformal_time_a1_a2
• Fixes and error checking for some obscure corner cases
• More robust to passing in non-contiguous or 32 bit vector arguments

1.3.2

• Source window functions now support bias(z) from Python interface (see sample notebook)
• get_partially_lensed_cls allows A_lens as function of L
• get_lensed_gradient_cls optionally supports using custom lensing spectrum input
• Added updated PRIMAT BBN interpolation table PRIMAT_Yp_DH_ErrorMC_2021.dat (thanks Cyril Pitrou)
• Added HMCode unit tests (thanks Alex Mead)
• Minor compatibility fixes

1.3.0

• Added HMCode 2020 and now default (thanks Alex Mead, arXiv:2009.01858)
• Raise error for w+wa>0 in dark energy models
• Added get_lensed_cls_with_spectrum and get_partially_lensed_cls for partially delensed and Alens-scaled lensed spectra
• Added correlation function and partial delensing examples to example notebook

1.2.0

• Quintessence dark energy support updated (from very old) and merged. Example implementation of early dark energy. In general, new models require deriving a new inherited quintessence class in Fortran and Python.
• Lensing and f_NL bispectrum code updated to work with latest version (no Python interface)
• Bug fixes for get_sigmaR and other small bug fixes/additional warnings.

1.1.3

• Correct get_valid_numerical_params
• Sympy 1.6 compatibility
• mathutils functions for polarization Pseudo-CL couplings and better doc

1.1.2

• get_sigmaR function
• get_valid_numerical_params to get list of valid parameter names
• Misc bug fixes
• Updated forutils to work around some recent gfortran version memory leak bugs

1.1.1

• Support setting zrei from set_cosmology
• Splined initial power spectrum now uses end values when out of range
• Add transfer function time sources examples to notebook
• Removed Python 2 support, code updates for Python 3.6+ (see python2 branch for old Python 2 version)

1.1

• Support for calculating only time source transfer functions, and then power spectra later. This allows calculating non-linear lensing results for different initial power spectrum and non-linear model parameters without recomputing the time transfer functions.
• Fix for Python raw lensing cross CMB output
• Allow k_per_logint to give denser k sampling even when used with non-linear lensing

1.0.12

• Support for wider range of input parameter values and more error propagation to Python
• Added k_hunit option to get_[non]linear_matter_power_spectrum
• get_matter_power_interpolator will now do log(-pk) interpolation for negative spectra
• Fix to assign Neff when omnuh2=0 (thanks @tilmantroester)
• Doc improvements for matter power variables, conda install, mathutils
• Fix for #66, #67
• Tweak to meta class to allow introspection of CAMB's Python classes to work
• Setting thetastar does not initialize reionization model or pk/windows (optimization, avoid errors)

1.0.9

• Fix for get_matter_power_interpolator extrapolation #61
• Fix for zstar calculation with tensors #62
• Tweaks for non-linear warnings and error handling