Difference between revisions of "C2"
| Line 2: | Line 2: | ||
| − | The main product to express cosmological constraints imposed by Planck data is a likelihood code. One of its by-products is the derived maximum-likelihood CMB spectrum, which is available for plotting purposes; see product | + | The main product to express cosmological constraints imposed by Planck data is a likelihood code. One of its by-products is the derived maximum-likelihood CMB spectrum, which is available for plotting purposes; see [[LFI_overview|product section]]. |
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 parameters paper. | 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 parameters paper. | ||
Revision as of 21:54, 4 July 2015
The main product to express cosmological constraints imposed by Planck data is a likelihood code. One of its by-products is the derived maximum-likelihood CMB spectrum, which is available for plotting purposes; see product section.
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 parameters 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
