Difference between revisions of "Lensing reconstructions 02.00"
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/project/projectdirs/cmbs4/reanalysis/phi_recons/02.00_carron_180920/plms_sepTP_apo_lmin200lmax3000_fsky5pc_cut10_180925 | /project/projectdirs/cmbs4/reanalysis/phi_recons/02.00_carron_180920/plms_sepTP_apo_lmin200lmax3000_fsky5pc_cut10_180925 | ||
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+ | There are 6 type of maps, labeled with | ||
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+ | sim_ptt_????_lmax3000.fits : lensing map from temperature only, simulation index ???? 0000 to 0099 | ||
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+ | sim_p_p_????_lmax3000.fits : lensing map from polarization only | ||
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+ | sim_p_????_lmax3000.fits : lensing map from temperature and polarization (MV) | ||
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+ | sim_xtt_????_lmax3000.fits : lensing curl map from temperature, useful for null tests | ||
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+ | sim_x_p_????_lmax3000.fits : lensing curl map from polarization | ||
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+ | sim_x_????_lmax3000.fits : lensing curl from temperature and polarization (MV) | ||
Revision as of 08:22, 27 September 2018
This page documents the 600 lensing maps (healpy alm fits file, lmax=3000) available at
/project/projectdirs/cmbs4/reanalysis/phi_recons/02.00_carron_180920/plms_sepTP_apo_lmin200lmax3000_fsky5pc_cut10_180925
There are 6 type of maps, labeled with
sim_ptt_????_lmax3000.fits : lensing map from temperature only, simulation index ???? 0000 to 0099
sim_p_p_????_lmax3000.fits : lensing map from polarization only
sim_p_????_lmax3000.fits : lensing map from temperature and polarization (MV)
sim_xtt_????_lmax3000.fits : lensing curl map from temperature, useful for null tests
sim_x_p_????_lmax3000.fits : lensing curl map from polarization
sim_x_????_lmax3000.fits : lensing curl from temperature and polarization (MV)
For illustration, the temperature (TT), polarization (PP) and Minimum Variance (MV) Wiener-filtered displacement reconstructions, together with the input, for realization 99:
The cross-correlation correlation to the input maps, as calculated across the entire patch is roughly like this:
The mean-field (here, contribution from the mask and noise anisotropies) has not been subtracted out from the maps on disk. The mean-field spectra look like this:
The mean-field subtraction can be performed subtracting the lensing reconstructed maps averaged over a subset of the simulations.