candl ================================================ Interface with candl. +-------------+----------------------------------------------+ | File | likelihood/candl/candl_cosmosis_interface.py | +-------------+----------------------------------------------+ | Attribution | Y. Omori | +-------------+----------------------------------------------+ | | L. Balkenhol | +-------------+----------------------------------------------+ | URL | https://github.com/Lbalkenhol/candl | +-------------+----------------------------------------------+ | Citations | https://doi.org/10.48550/arXiv.2401.13433 | +-------------+----------------------------------------------+ Interface to candl. Assumptions ----------- - candl python module Setup Parameters ---------------- .. list-table:: :header-rows: 1 * - Name - Type - Default - Description * - data_set - str - - The data set to use * - variant - str - None - Variant of the data set requested, if applicable. * - lensing - bool - True - Lensing likelihood (or primary CMB). * - feedback - bool - True - Whether to generate feedback from the likelihood initialisation. * - data_selection - any - ... - Further data selection * - clear_1d_internal_priors - bool - True - Delete all 1d Gaussian priors implemented in candl. * - clear_nd_internal_priors - bool - False - Delete all >1d Gaussian priors implemented in candl. Beware: CosmoSIS does not have support for higher-dimensional Gaussian priors. * - force_ignore_transformations - str - None - Backdoor to explicitly ignore certain transformations in the data model. See candl documentation for more information. Input values ---------------- .. list-table:: :header-rows: 1 * - Section - Name - Type - Default - Description * - cmb_cl - ell - real 1d - - CMB power spectrum ell values of other inputs * - - tt - real 1d - - Lensed CMB temperature power spectrum in ell(ell+1)/2pi units * - - te - real 1d - - Lensed CMB temperature-E-mode polarization cross power spectrum in ell(ell+1)/2pi units * - - ee - real 1d - - Lensed CMB E-mode polaration power spectrum in ell(ell+1)/2pi units * - - bb - real 1d - - Lensed CMB B-mode polaration power spectrum in ell(ell+1)/2pi units * - - pp - real 1d - - CMB lensing phi-phi power spectrum in ell(ell+1)/2pi units Output values ---------------- .. list-table:: Output values :header-rows: 1 * - Section - Name - Type - Description * - likelihoods - candl_like - real - candl likelihood