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 Model 92, all frequencies and both apodized masks fsky25 and fsky50.

Sevem Bandpowers for Model 92, all frequencies, for mask fsky50, vs the input model (solid orange line) for lmax=1000

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Sevem Bandpowers for Model 92, all frequencies, for mask fsky50, vs the input model (solid orange line) for lmax=300

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Sevem Bandpowers for Model 92, all frequencies, for mask fsky25, vs the input model (solid orange line) for lmax=1000

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Sevem Bandpowers for Model 92, all frequencies, for mask fsky25, vs the input model (solid orange line) for lmax=300

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