Zobrazeno 1 - 10
of 140
pro vyhledávání: '"Odenwald S"'
Publikováno v:
Astrophys.J. 579 (2002) L53-L57
We report first results for the cosmic infrared background (CIB) fluctuations at 1.25, 1.65 and 2.17 micron obtained from long exposures constructed from 2MASS standard star fields. We have co-added and analyzed scans from one such field with a total
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210083
Publikováno v:
Astrophys.J. 583 (2003) 535-550
This is one of two papers in which we report the detection of structure in the cosmic infrared background (CIB) between 1.25 - 2.2 micron through the use of data from the Two Micron Sky Survey (2MASS). This paper concentrates on data assembly, analys
Externí odkaz:
http://arxiv.org/abs/astro-ph/0210084
The cosmic infrared background (CIB) radiation is the cosmic repository for energy release throughout the history of the universe. Using the all-sky data from the COBE DIRBE instrument at wavelengths 1.25 - 100 mic we attempt to measure the CIB fluct
Externí odkaz:
http://arxiv.org/abs/astro-ph/9908304
We discuss a new method of estimating the cosmic infrared background (CIB) from the spatial properties of infrared maps and give the limits on the CIB from applying it to the COBE/DIRBE maps. The strongest limits are obtained at mid- to far-IR where
Externí odkaz:
http://arxiv.org/abs/astro-ph/9701216
Publikováno v:
Astrophys.J.473:L9,1996
We measure the smoothness of the infrared sky using the COBE DIRBE maps, and obtain interesting limits on the production of the diffuse cosmic infrared background (CIB) light by matter clustered like galaxies. The predicted fluctuations of the CIB wi
Externí odkaz:
http://arxiv.org/abs/astro-ph/9610051
Publikováno v:
Astrophys.J. 470 (1996) 681
This paper is devoted to studying the CIB through its correlation properties. We studied the limits on CIB anisotropy in the near IR (1.25, 2.2, and 3.5 \um, or $J,\;K,\;L$) bands at a scale of 0.7\deg\ using the COBE\footnote{ The National Aeronauti
Externí odkaz:
http://arxiv.org/abs/astro-ph/9604182
The cosmic infrared background from galaxies should have a minimum fluctuation of the order of 10\% on angular scales probed by the DIRBE (Diffuse Infrared Background Experiment) on board COBE (Cosmic Background Explorer). We present the theoretical
Externí odkaz:
http://arxiv.org/abs/astro-ph/9604181
We outline a new method for estimating the cosmic infrared background using the spatial and spectral correlation properties of infrared maps. The cosmic infrared background from galaxies should have a minimum fluctuation of the order of 10\% on angul
Externí odkaz:
http://arxiv.org/abs/astro-ph/9604180
Publikováno v:
Der Unfallchirurg; 20240101, Issue: Preprints p1-7, 7p
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