Difference between revisions of "Additional angular power spectra"

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= Detset Angular Power spectra =
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While the HFI is not providing sky maps obtained with different subsets of the detectors in a given frequency channel (see [[Frequency  Maps#Detector-set maps|Detset maps]]), it provides auto-spectra and cross-spectra derived from these maps. 
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<span style="color:red">
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'''Outstanding:'''
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* <span style="color:red">KB and/or EFH to add description of auto & cross spectra and of the associated covariance matrices
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* <span style="color:red">AMo to add description of file with sample header
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</span>
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[[Category:PLA contents]]
 
[[Category:PLA contents]]

Revision as of 10:45, 22 January 2013

Detset Angular Power spectra[edit]

While the HFI is not providing sky maps obtained with different subsets of the detectors in a given frequency channel (see Detset maps), it provides auto-spectra and cross-spectra derived from these maps.

Outstanding:

  • KB and/or EFH to add description of auto & cross spectra and of the associated covariance matrices
  • AMo to add description of file with sample header

(Planck) High Frequency Instrument