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 compare the Bandpowers and residuals for SEVEM maps for Foreground Models 90, 91 and 92.

Band Powers (BP) and uncertainties for SEVEM maps simulated considering the following foreground models: 90,91 and 92 (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 (Data and Noise) and Masks located at nersc:

/project/projectdirs/pico/reanalysis/compsepmaps/sevem_04.00_180815/ - Model 90
Bandpowers estimated for (non-apodized) mask mask0.15_pol_sm7deg_nu0p45_up512.fits

/project/projectdirs/pico/reanalysis/compsepmaps/sevem_04.00_181011/MODEL90.91/ - Model 91
Bandpowers estimated for apodized masks: mask_m91_fsky25.fits and mask_m91_fsky50.fits

/project/projectdirs/pico/reanalysis/compsepmaps/sevem_04.00_181011/MODEL90.92/ - Model 92
Bandpowers estimated for apodized masks: mask_m92_fsky25.fits and mask_m92_fsky50.fits

beam window function: /project/projectdirs/pico/reanalysis/powspecpars/Bl bl_gauss_6.2arcmin_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/

BB bandpowers for the 155GHz clean sevem map for foreground models 90, 91 and 92.
Note that the mask used for model 90 is not apodized while both masks for models 91 and 92 are apodized
Next we will replace by the BP estimated for the apodized mask and/or full-sky.

BB lmax=1000		BB lmax=300
m90 non-apodized mask		m90 apodized mask

Sevem Bandpowers for Maps generated considering the foreground models: 90, 91 and 92; 155GHz, for non-apodized mask (model 90) and fsky25 and fsky50 (models 91 and 92), vs the input model (solid orange line) for lmax=1000

TT		TE

EE		BB

Sevem Bandpowers for Maps generated considering the foreground models: 90, 91 and 92; 155GHz, for non-apodized mask (model 90) and fsky25 and fsky50 (models 91 and 92), vs the input model (solid orange line) for lmax=300

TT		TE

EE		BB