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 Model 90, Model 91 and Model 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 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