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<i>Planck</i>intermediate results. XXII. Frequency dependence of thermal emission from Galactic dust in intensity and polarization
Planck has mapped the intensity and polarization of the sky at microwave frequencies with unprecedented sensitivity. We use these data to characterize the frequency dependence of dust emission. We make use of the Planck 353 GHz I, Q, and U Stokes maps as dust templates, and cross-correlate them with the …