Fig. 8 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. 8.

Correlations of Fig. 7 averaged within bins along the fit lines. The bin boundaries used are perpendicular to the fit lines on plots where each variable is divided by its mean measurement error. The error bars are parallel to the bin boundaries and show the standard error of the mean for the data within each bin.

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