# Difference between revisions of "C2"

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The main product to express cosmological constraints posed by Planck data is a likelihood code. One of its by-product is the derived maximum-likelihood CMB spectrum, which is available for plotting purposes; see product page. | The main product to express cosmological constraints posed by Planck data is a likelihood code. One of its by-product is the derived maximum-likelihood CMB spectrum, which is available for plotting purposes; see product page. | ||

− | The likelihood code itself will be released together with the corresponding "CMB power spectra and likelihood" paper; however, a short summary of the approach (similar to that used | + | The likelihood code itself will be released together with the corresponding "CMB power spectra and likelihood" paper {{PlanckPapers|planck2014-a13||Planck-2015-A13}}; however, a short summary of the approach (similar to that used in 2013) is already available in the 2015 release parameter paper. |

+ | == References == | ||

+ | <references /> | ||

[[Category:HFI/LFI joint data processing|004]] | [[Category:HFI/LFI joint data processing|004]] |

## Revision as of 18:14, 4 February 2015

The main product to express cosmological constraints posed by Planck data is a likelihood code. One of its by-product is the derived maximum-likelihood CMB spectrum, which is available for plotting purposes; see product page.

The likelihood code itself will be released together with the corresponding "CMB power spectra and likelihood" paper Planck-2015-A13^{[1]}; however, a short summary of the approach (similar to that used in 2013) is already available in the 2015 release parameter paper.

## References[edit]

- ↑
**Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of cosmological parameters**, Planck Collaboration, 2016, A&A, 594, A11.

Cosmic Microwave background