Fig. 17 from The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. III. Separation of Galactic Emission from the Infrared Sky Brightness

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The COBE Diffuse Infrared Background Experiment Search for the Cosmic Infrared Background. III. Separation of Galactic Emission from the Infrared Sky Brightness

Authors: R. G. Arendt, N. Odegard, J. L. Weiland, T. J. Sodroski, M. G. Hauser, E. Dwek, T. Kelsall, S. H. Moseley, R. F. Silverberg, D. Leisawitz, K. Mitchell, W. T. Reach, and E. L. Wright

Arendt et al. 1998 The Astrophysical Journal 508 74.

Provider: AAS Journals

Caption: Fig. 17.

Map of the reddening‐free parameter, Q(1.25, 2.2, 3.5). Midlatitude structures near (l, b) = (90°, +20°) and (270°, −20°) can be seen to correlate with ISM emission (e.g., the 240 μm emission in Fig. 1). Residual IPD errors cause artifacts (extended blue regions) at low ecliptic latitudes.

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