Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.7203j&link_type=abstract
American Astronomical Society, 197th AAS Meeting, #72.03; Bulletin of the American Astronomical Society, Vol. 32, p.1515
Astronomy and Astrophysics
Astronomy
Scientific paper
The cosmic infrared background (CIRB) is the sum total of the redshifted and reprocessed radiation from the era of galaxy formation. The intensity and spectrum of the CIRB provide information about the history of star formation, the history of galaxy formation, and the presence or absence of dust in early galaxies. We present tentative detections of the CIRB at 2.2 microns for 10 3x3 degree patches of sky at high galactic latitudes. These detections are derived from the low-resolution maps of the infrared sky produced by the Diffuse Infrared Background Experiment (DIRBE) on the Cosmic Background Explorer (COBE). The main problem in determining the CIRB from these maps is the removal of foreground sources. Zodiacal light is subtracted using the zodiacal light model of Kelsall et al. (1998,ApJ,508,44) and Wright (1997,BAAS,29,1354). Stars of our galaxy with 4
Johnson Benjamin D.
Wright Louis E.
No associations
LandOfFree
Tentative Detection of the Cosmic Infrared Background at 2.2 Microns does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Tentative Detection of the Cosmic Infrared Background at 2.2 Microns, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tentative Detection of the Cosmic Infrared Background at 2.2 Microns will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1725031