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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. 19.

Correlation plots of data for the lines of sight in samples 1, 2, and 4. The error bars show 1 σ measurement errors. The line shown in each panel is an unweighted least‐squares fit that minimizes the residuals in the ordinate. (a) Correlation of 100 μm data with H I column density. (b) Correlation of extinction‐corrected Hα intensity (for samples 1 and 2) or H II column density (for sample 4) with H I column density. (c) Correlation of residuals from the fit of (a) with residuals from the fit of (b).

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