We report here the Band Power Spectra and parameters estimated for the component separation methods applied to Simulated data. For each method we estimate the full sky band power spectra with Xfaster, propagate to parameters with a Gaussian correlated Likelihood, and sample parameters with CosmoMC, marginalizing over tailored foreground residual templates. In addition we consider a hybrid likelihood: BFlike (pixel based likelihood) at low-l and XFlike (Xfaster likelihood) at high-l.

We show Bandpowers and residuals for SEVEM maps for Model91.

Band Powers (BP) and uncertainties for SEVEM combined map, case 91.00 (first panel).
Also shown are the residuals of the estimated BP and the input spectra used to simulate the input maps (second panel).
The BP was estimated with XFpipe.

maps and mask are located at:

observation: /project/projectdirs/pico/reanalysis/compsepmaps/sevem_04.00_181011/MODEL90.91/data_combined_90_108_129_155_fwf15.0d0.fits

noise: /project/projectdirs/pico/reanalysis/compsepmaps/sevem_04.00_181011/MODEL90.91/noise_combined_90_108_129_155_fwf15.0d0.fits

mask: /project/projectdirs/pico/reanalysis/compsepmaps/sevem_04.00_181011/MODEL90.91/ mask_m91_fsky50.fits - fsky50
and
/project/projectdirs/pico/reanalysis/compsepmaps/sevem_04.00_180815/
mask0.15_pol_sm7deg_nu0p45_up512_sm7deg_nu0p57_apocos5pix.fits - maskapo
mask0.15_pol_sm7deg_nu0p45_up512_apocos5pix.fits - maskapo_v1
mask0.15_pol_sm7deg_nu0p45_up512.fits - mask

beam window function: /project/projectdirs/pico/reanalysis/powspecpars/Bl bl_gauss_15.0arcmin_comb_TP.dat

Binning_scheme: CTP: /project/projectdirs/pico/reanalysis/powspecpars/bins CTP_bin_TT; CTP_bin_TE; CTP_bin_EE; CTP_bin_BB

input spectra: /project/projectdirs/pico/sky_yy/cmb/cls/ ffp10_lensedCls.dat

Spectra is located at /project/projectdirs/pico/reanalysis/powspecpars/sevem_04.00_180815_180921/spectra/

sevem_model91_comb_15arcmin_uK_mask_l1500_Gfg.newdat
sevem_model91_comb_15arcmin_uK_maskapo_l1500_Gfg.newdat