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 16:49, 21 January 2015
Overview
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
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 CMBCosmic Microwave background 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 CMBCosmic Microwave background 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 FITSFlexible Image Transfer Specification format alm, with [math] L_{\rm max} = 2048 [/math] | Contains the estimated lensing convergence [math] \hat{\kappa}_{LM} = \frac{1}{2} L(L+1)\hat{\phi}_{LM} [/math]. |
mask.fits.gz | HEALPIX FITSFlexible Image Transfer Specification format map, with [math] N_{\rm side} = 2048 [/math] | Contains the lens reconstruction analysis mask. |
nlkk.dat | ASCII text file, with columns = ([math]L[/math], [math]N_L [/math], [math]C_L+N_L[/math]) | The approximate noise [math]N_L[/math] (and signal+noise, [math]C_L+N_L[/math]) power spectrum of [math] \hat{\kappa}_{LM} [/math], for the fiducial cosmology used in ^{[1]}. |
Compton parameter map
TBW
References
- ↑ ^{1.0} ^{1.1} ^{1.2}