Difference between revisions of "Additional angular power spectra"
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'''Outstanding:''' | '''Outstanding:''' | ||
| − | * <span style="color:red"> | + | * <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. | ||
</span> | </span> | ||
[[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
