Difference between revisions of "C2"
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| − | + | {{DISPLAYTITLE:CMB power spectra}} | |
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| − | + | 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 [[Mission_products|product section]]. | |
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| + | The likelihood code itself was released together with the corresponding "CMB power spectra and likelihood" paper ({{PlanckPapers|planck2014-a13}}). A short summary of the approach (similar to that used in 2013) is also available in the 2015 release parameters paper ({{PlanckPapers|planck2014-a15}}). | ||
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| + | == References == | ||
| + | <references /> | ||
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| + | [[Category:HFI/LFI joint data processing|004]] | ||
Latest revision as of 06:35, 12 January 2017
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 was released together with the corresponding "CMB power spectra and likelihood" paper (Planck-2015-A11[1]). A short summary of the approach (similar to that used in 2013) is also available in the 2015 release parameters paper (Planck-2015-A13[2]).
References[edit]
- ↑ Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of cosmological parameters, Planck Collaboration, 2016, A&A, 594, A11.
- ↑ Planck 2015 results. XIII. Cosmological parameters, Planck Collaboration, 2016, A&A, 594, A13.
Cosmic Microwave background
