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BICEP2 module
Compute the likelihood of the supplied CMB power spectra
Name: BICEP2
File: cosmosis-standard-library/likelihood/bicep2/bicep_interface.py
Version: 20140314
Author(s):
- BICEP2 Team
URL: http://bicepkeck.org
Cite:
Rules:
Assumptions:
- CAMB or other CMB code must be set up to do lensing and include high k modes
- BICEP2 2014-03-14 dataset
Explanation
The 2014 BICEP2 results are a detection of cosmological B-modes
on the scales that indicate a primordial gravitational wave bump.
This module wraps the likelihood code released by the BICEP2 team.
##Parameters
These parameters can be set in the module's section in the ini parameter file.
If no default is specified then the parameter is required.
Parameter | Description |
---|---|
##Inputs
These parameters and data are inputs to the module, either supplied as parameters by the sampler or computed by some previous module. They are loaded from the data block.
Section | Parameter | Description |
---|---|---|
cmb_cl | ell | 1D integers, Angular wavenumbers for the input spectra |
EE | 1D real, EE CMB power spectrum, at wavenumbers from ell | |
BB | 1D real, BB CMB power spectraum, at wavenumbers from ell |
##Outputs
These parameters and data are computed as outputs from the module
Section | Parameter | Description |
---|---|---|
likelihoods | BICEP_LIKe | real, likelihood of supplied spectra from BICEP2 |
Updated