Difference between revisions of "Lensing reconstructions 02.00"
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sim_x_????_lmax3000.fits : lensing curl from temperature and polarization (MV) | sim_x_????_lmax3000.fits : lensing curl from temperature and polarization (MV) | ||
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| + | The maps were built using the quadratic estimator implementation described [https://arxiv.org/abs/1807.06210 in the 2018 CMB lensing paper], | ||
| + | with the exception of the filtering, which is isotropic after application of a slightly apodized mask. The filtering uses | ||
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[[File:recmaps_cmbs4_apo.png]] | [[File:recmaps_cmbs4_apo.png]] | ||
| + | == Reconstruction parameters == | ||
| + | == Fidelity to the input == | ||
The cross-correlation correlation to the input maps, as calculated across the entire patch is roughly like this: | The cross-correlation correlation to the input maps, as calculated across the entire patch is roughly like this: | ||
[[File:cmbs4rho.png]] | [[File:cmbs4rho.png]] | ||
| + | == Mean-fields == | ||
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 (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: | ||
Revision as of 08:29, 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)
The maps were built using the quadratic estimator implementation described in the 2018 CMB lensing paper, with the exception of the filtering, which is isotropic after application of a slightly apodized mask. The filtering uses
For illustration, the temperature (TT), polarization (PP) and Minimum Variance (MV) Wiener-filtered displacement reconstructions, together with the input, for realization 99:
Reconstruction parameters
Fidelity to the input
The cross-correlation correlation to the input maps, as calculated across the entire patch is roughly like this:
Mean-fields
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.
