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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
