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arXiv:astro-ph/0004192 (astro-ph)
[Submitted on 13 Apr 2000 (v1), last revised 31 Jan 2001 (this version, v3)]

Title:DIRBE Minus 2MASS: Confirming the Cosmic Infrared Background at 2.2 Microns

Authors:E. L. Wright (UCLA)
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Abstract: Stellar fluxes from the 2MASS catalog are used to remove the contribution due to Galactic stars from the intensity measured by DIRBE in four regions in the North and South Galactic polar caps. After subtracting the interplanetary and galactic foregrounds, a consistent residual intensity of 14.8 +/- 4.6 kJy/sr or 20.2 +/- 6.3 nW/m^2/sr at 2.2 microns is found. At 1.25 microns the residuals show more scatter and are a much smaller fraction of the foreground, leading to a weak limit on the CIRB of 12.0 +/- 6.8 kJy/sr or 28.9 +/- 16.3 nW/m^2/sr (1 sigma).
Comments: ApJ in press. 14 pages Latex with 7 included figures. accepted version with 1 new figure
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/0004192
  (or arXiv:astro-ph/0004192v3 for this version)
  https://doi.org/10.48550/arXiv.astro-ph/0004192
Related DOI: https://doi.org/10.1086/320942

Submission history

From: Edward L. Wright [view email]
[v1] Thu, 13 Apr 2000 21:03:47 UTC (31 KB)
[v2] Tue, 27 Jun 2000 01:31:44 UTC (39 KB)
[v3] Wed, 31 Jan 2001 18:20:26 UTC (43 KB)
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