Difference between revisions of "Frequency map angular power spectrum"
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==CMB angular power spectra== | ==CMB angular power spectra== | ||
| − | + | Auto and cross angular power spectra per frequency are provided in the Planck Legacy Archive with the following file structure: | |
| + | <span style="color:red">to be written by A. Moneti</span> | ||
| − | + | They were obtained by Spice (run 1731634056805856210) with the Galactic and point sources masks | |
| + | /data/dmc/MISS03/DATA/gpe_mask/mask_2_apo120, | ||
| + | /data/dmc/MISS03/DATA/MASK_2048_GALACTIC/mask_L3_DX9_100-353_apo30, | ||
| + | /data/dmc/MISS03/DATA/MASK_2048_GALACTIC/mask_SZ_ERCSC_apo30, | ||
| + | respectively apodized at 120, 30 and 30 arcmin. | ||
| − | + | The covariance matrix only describes the statistical correlation induced by the sample variance and cut sky, | |
| + | using the formalism described in Efstathiou ?? | ||
[[Category:Mission science products]] | [[Category:Mission science products]] | ||
Revision as of 15:10, 8 February 2013
CMB angular power spectra[edit]
Auto and cross angular power spectra per frequency are provided in the Planck Legacy Archive with the following file structure: to be written by A. Moneti
They were obtained by Spice (run 1731634056805856210) with the Galactic and point sources masks /data/dmc/MISS03/DATA/gpe_mask/mask_2_apo120, /data/dmc/MISS03/DATA/MASK_2048_GALACTIC/mask_L3_DX9_100-353_apo30, /data/dmc/MISS03/DATA/MASK_2048_GALACTIC/mask_SZ_ERCSC_apo30, respectively apodized at 120, 30 and 30 arcmin.
The covariance matrix only describes the statistical correlation induced by the sample variance and cut sky, using the formalism described in Efstathiou ??
Cosmic Microwave background
Sunyaev-Zel'dovich
Early Release Compact Source Catalog
