Releases: cmbant/CAMB
Releases Β· cmbant/CAMB
1.5.7
1.5.5
1.5.3
1.5.1
1.5.0
- Fixed bug calculating Cl from time sources that affected iterated use in Cobaya
- Increase max transfer redshifts to 256
- Added min_l_logl_sampling parameter to set_accuracy (to set lowest multipole at which sparse log-L sampling is used)
- Added sample transfer function animations to the end of the example notebook
1.4.0
- Updated numerical constants, use latest definitions for Megaparsec, and calculate times in Julian giga-years
- Updated default nnu to 3.044 (from 3.046)
- Updated default BBN model (for helium abundance) to PRIMAT2021
- Support general bias(k,z) for source window functions
- Fix for HMcode-2020 feedback at low k
- Fix get_matter_power_spectrum for cross-spectra
- Allow read_ini to load directly from a URL
- Minor code tidies
These changes do change numerical results, but only at a level that is irrelevant for near-future observations. But some of the higher-precision unit tests also had to be updated.
1.3.6
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