Additional angular power spectra
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 Detset maps), it provides auto-spectra and cross-spectra derived from these maps.
- 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