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.
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{{DISPLAYTITLE:CMB power spectra}}
  
NB: This is very much a scientific product, whose development status will be described in a dedicated talk at the review.
 
  
==CLIK - The Planck C(l) LIKelihood code ==
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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.
  
==Current Best-fit CMB spectrum==
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The likelihood code itself will be released together with the corresponding "CMB power spectra and likelihood" paper {{PlanckPapers|planck2014-a13}}; however, a short summary of the approach (similar to that used in 2013) is already available in the 2015 release parameter paper.
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== References ==
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<references />
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[[Category:HFI/LFI joint data processing|004]]

Latest revision as of 15:17, 26 September 2016


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-A11[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]

Cosmic Microwave background