Fsky

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Dependence of BB power of dust on sky fraction for different levels of apodization. From top to bottom, no apodization, apodized with Gaussian profile with 1, 2, 5 degrees FWHM. Red shows halfmission cross-spectra, blue shows detector set cross-spectra.

Dust.png

Dependence of BB power of synchrotron emission on sky fraction for different levels of apodization. From top to bottom, no apodization, apodized with Gaussian profile with 1, 2, 5 degrees FWHM.

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Dependence of BB power of synchrotron component correlated with dust on sky fraction for different levels of apodization. From top to bottom, no apodization, apodized with Gaussian profile with 1, 2, 5 degrees FWHM.

Corr.png

Dependence of BB power on sky fraction for different types of apodization. Lower curve corresponds to apodization with Gaussian with 5 degree FWHM, upper curve corresponds to apodization described in Planck likelihood paper.

Apod.png

Dependence of BB power on sky fraction for apodization chosen to match Planck's apodization and comparison to PXXX (shown in orange).

PXXX.png