DERIVATION OF A LARGE ISOTOPIC DIFFUSE SKY EMISSION COMPONENT AT 1.25 AND 2.2 mu m FROM THE COBE/DIRBE DATA

作者：Sano K^*; Kawara K; Matsuura S; Kataza H; Arai T; Matsuoka Y

来源：Astrophysical Journal, 2015, 811(2): 77.

DOI：10.1088/0004-637X/811/2/77

• cosmic background radiation
• dust, extinction
• infrared: ISM
• infrared: stars
• scattering
• zodiacal dust

Using all-sky maps obtained with COBE/DIRBE, we reanalyzed the diffuse sky brightness at 1.25 and 2.2 mu m, which consists of zodiacal light, diffuse Galactic light (DGL), integrated starlight (ISL), and isotropic emission including the extragalactic background light. Our new analysis including an improved estimate of the DGL and the ISL with the 2MASS data showed that deviations of the isotropic emission from isotropy were less than 10% in the entire sky at high Galactic latitude (vertical bar b vertical bar > 35 degrees). We derived the DGL to 100 mu m brightness ratios of similar to 4.79 and similar to 1.49 n W m(-2) MJy(-1) at 1.25 and 2.2 mu m, respectively. The result of our analysis revealed a significantly large isotropic component at 1.25 and 2.2 mu m with intensities of 60.15 +/- 16.14 and 27.68 +/- 6.21 n W m(-2) sr(-1), respectively. This intensity is larger than the integrated galaxy light, upper limits from gamma-ray observation, and potential contribution from exotic sources (i.e., Population III stars, intrahalo light, direct collapse black holes, and dark stars). We therefore conclude that the excess light may originate from the local universe: the Milky Way and/or the solar system.

• 出版日期2015-10-1
• 单位中国科学院国家天文台