Dust emission from Planck

Tuhin Ghosh (l’Institut d’Astrophysique Spatiale, Orsay)

January 12, 2015

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Abstract: The Planck satellite has mapped the microwave sky (from 30 to 857 GHz) with unprecedented sensitivity and angular resolution. This wealth of data shed new lights on the polarization of the CMB emission and Galactic foregrounds, especially that of the thermal emission from the dust grains. I will present the results related to the dust emission from the Planck data.