Difference between revisions of "Additional angular power spectra"
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| + | = Detset Angular Power spectra = | ||
| + | |||
| + | 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. | ||
| + | |||
| + | <span style="color:red"> | ||
| + | '''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">AMo to add description of file with sample header | ||
| + | </span> | ||
| + | |||
[[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
