Statistical simulations of the dust foreground to cosmic microwave background polarization

F. Vansyngel; F. Boulanger; T. Ghosh; B. Wandelt; J. Aumont; A. Bracco; F. Levrier; P. G. Martin; L. Montier

doi:10.1051/0004-6361/201629992

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Volume 603 (July 2017)

A&A, 603 (2017) A62

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This article has an erratum: [https://doi.org/10.1051/0004-6361/201629992e]

Fig. 8

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High resolution power spectra on the LR63 region; simulation vs. data. From top to bottom: TE, EE, and BB power spectra of the Planck353GHz, CMB-corrected maps (black), and one high resolution (N_side = 2048, FWHM = 10′) realization of the model (red).

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