Difference between revisions of "Specially processed maps"
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== IRAM Maps of the Crab nebula == | == IRAM Maps of the Crab nebula == | ||
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See README in the tarball for full details. These data were used in{{BibCite|aumont2010}} | See README in the tarball for full details. These data were used in{{BibCite|aumont2010}} | ||
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==References== | ==References== |
Revision as of 15:49, 21 January 2015
Overview[edit]
This section describes products that require special processing. Only one such product is available at this time; this section will be expanded with time as more products are added.
Lensing map[edit]
We distribute the minimum-variance (MV) lensing potential estimate presented in [1] as part of the 2014 data release. This map represents an estimate of the CMB lensing potential on approximately 70% of the sky, and also forms the basis for the Planck 2014 lensing likelihood. It is produced using filtered temperature and polarization data from the SMICA DX11 CMB map; its construction is discussed in detail in [1].
The estimate is contained in a single gzipped tarball named COM_CompMap_Lensing_2048_R0.00.tgz. Its contents are described below.
Filename | Format | Description |
---|---|---|
dat_klm.fits | HEALPIX FITS format alm, with | Contains the estimated lensing convergence | .
mask.fits.gz | HEALPIX FITS format map, with | Contains the lens reconstruction analysis mask. |
nlkk.dat | ASCII text file, with columns = ( | , , )The approximate noise [1]. | (and signal+noise, ) power spectrum of , for the fiducial cosmology used in
Compton parameter map[edit]
TBW
References[edit]
Cosmic Microwave background
Flexible Image Transfer Specification