Difference between revisions of "Additional angular power spectra"

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'''Outstanding:'''
 
'''Outstanding:'''
* <span style="color:red">KB and/or EFH to add description of auto & cross spectra and of the associated covariance matrices
+
* <span style="color:red">EFH to add the purpose of these spectra and of the associated covariance matrices, and a description of how they are obtained, including the inputs used to build them (maps, beams, mask),
* <span style="color:red">AMo to add description of file with sample header
+
* <span style="color:red">AMo to add description of FITS file with sample header.
 +
* <span style="color:red">NB. contrary to the R1.00 (pre-)delivery, in the R1.10 final delivery each spectrum and associated covar matrix will be packaged together in a single file.
 
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[[Category:PLA contents]]
 
[[Category:PLA contents]]

Revision as of 11:12, 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:

  • EFH to add the purpose of these spectra and of the associated covariance matrices, and a description of how they are obtained, including the inputs used to build them (maps, beams, mask),
  • AMo to add description of FITS file with sample header.
  • NB. contrary to the R1.00 (pre-)delivery, in the R1.10 final delivery each spectrum and associated covar matrix will be packaged together in a single file.

(Planck) High Frequency Instrument

Flexible Image Transfer Specification