Fig. 7 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. 7.

Correlation of DIRBE 100 μm intensities after subtraction of IPD emission with H I column density for (a) the north ecliptic pole region, (b) a region of low H I column density in Ursa Major, and (c) the region of high‐latitude sky (|b| > 25°, |β| > 25°) covered by the Bell Laboratories H I survey. The solid lines show fits to the data as described in § 5.2.1. Data above the short diagonal lines were excluded from the fitting.

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