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 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]].
  
==Current Best-fit CMB spectrum==
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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 ==
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<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]

Cosmic Microwave background