Supplementary materials for Astronomy and Astrophysics article: "Far-infrared to centimeter emission of very nearby galaxies with archival data" by Correia. L et al.
Abstract
Maps of the galaxies in 18 photometric bands of COBE-DIRBE, IRAS, \textit{Planck} and WMAP from 97 µm to 1.3cm, before and after the subtraction of the foreground and background sources. The solid and dashed white lines delineate the on-source and background regions used for the aperture photometry, respectively.
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-25° -30° -35° -40° Galactic Latitude COBE-DIRBE 97 m 0 100000 MJy/sr (×10 3) IRAS 100 m 0 100000 MJy/sr (×10 3) COBE-DIRBE 140 m 0 100000 MJy/sr (×10 3) -25° -30° -35° -40° Galactic Latitude COBE-DIRBE 240 m 0 50000 MJy/sr (×10 3) Planck 350 m 0 20000 MJy/sr (×10 3) Planck 500 m 0 5000 MJy/sr (×10 3) -25° -30° -35° -40° Galactic Latitude Planck 850 m 0 2000 MJy/sr (×10 3) Planck 1.3 mm 0 250 MJy/sr (×10 3) Planck 2.1 mm 0 100 MJy/sr (×10 3) -25° -30° -35° -40° Galactic Latitude Planck 3 mm 0 50 MJy/sr (×10 3) WMAP 3.2 mm 0 50 MJy/sr (×10 3) Planck 4.3 mm 0 100 MJy/sr (×10 3) -25° -30° -35° -40° Galactic Latitude WMAP 4.9 mm 0 100 MJy/sr (×10 3) Planck 6.8 mm 0 100 MJy/sr (×10 3) WMAP 7.3 mm 0 100 MJy/sr (×10 3) -25° -30° -35° -40° Galactic Latitude WMAP 9.1 mm 0 100 MJy/sr (×10 3) Planck 10 mm 0 100 MJy/sr (×10 3) WMAP 13 mm 0 100 MJy/sr (×10 3)