candl
Interface with candl.
File |
likelihood/candl/candl_cosmosis_interface.py |
Attribution |
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URL |
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Citations |
Interface to candl.
Assumptions
candl python module
Setup Parameters
Name |
Type |
Default |
Description |
|---|---|---|---|
data_set |
str |
The data set to use |
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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
Section |
Name |
Type |
Default |
Description |
|---|---|---|---|---|
cmb_cl |
ell |
real 1d |
CMB power spectrum ell values of other inputs |
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tt |
real 1d |
Lensed CMB temperature power spectrum in ell(ell+1)/2pi units |
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te |
real 1d |
Lensed CMB temperature-E-mode polarization cross power spectrum in ell(ell+1)/2pi units |
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ee |
real 1d |
Lensed CMB E-mode polaration power spectrum in ell(ell+1)/2pi units |
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bb |
real 1d |
Lensed CMB B-mode polaration power spectrum in ell(ell+1)/2pi units |
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pp |
real 1d |
CMB lensing phi-phi power spectrum in ell(ell+1)/2pi units |
Output values
Section |
Name |
Type |
Description |
|---|---|---|---|
likelihoods |
candl_like |
real |
candl likelihood |