Dissecting the cosmic infra-red background with Herschel/PEP

作者：Berta S^*; Magnelli B; Lutz D; Altieri B; Aussel H; Andreani P; Bauer O; Bongiovanni A; Cava A; Cepa J; Cimatti A; Daddi E; Dominguez H; Elbaz D; Feuchtgruber H; Schreiber N M Foerster; Genzel R; Gruppioni C; Katterloher R; Magdis G; Maiolino R; Nordon R; Perez Garcia A M; Poglitsch A; Popesso P; Pozzi F; Riguccini L; Rodighiero G; Saintonge A; Santini P; Sanchez Portal M; Shao L; Sturm E; Tacconi L J; Valtchanov I

来源：Astronomy & Astrophysics, 2010, 518: L30.

DOI：10.1051/0004-6361/201014610

• infrared: diffuse background
• infrared: galaxies
• cosmic background radiation
• galaxies: statistics
• galaxies: evolution

The constituents of the cosmic IR background (CIB) are studied at its peak wavelengths (100 and 160 mu m) by exploiting Herschel/PACS observations of the GOODS-N, Lockman Hole, and COSMOS fields in the PACS evolutionary probe (PEP) guaranteed-time survey. The GOODS-N data reach 3 sigma depths of similar to 3.0 mJy at 100 mu m and similar to 5.7 mJy at 160 mu m. At these levels, source densities are 40 and 18 beams/source, respectively, thus hitting the confusion limit at 160 mu m. Differential number counts extend from a few mJy up to 100-200 mJy, and are approximated as a double power law, with the break lying between 5 and 10 mJy. The available ancillary information allows us to split number counts into redshift bins. At z <= 0.5 we isolate a class of luminous sources (L(IR) similar to 10(11) L(circle dot)), whose SEDs resemble late-spiral galaxies, peaking at similar to 130 mu m restframe and significantly colder than what is expected on the basis of pre-Herschel models. By integrating number counts over the whole covered flux range, we obtain a surface brightness of 6.36 +/- 1.67 and 6.58 +/- 1.62 [nW m(-2) sr(-1)] at 100 and 160 mu m, resolving similar to 45% and similar to 52% of the CIB, respectively. When stacking 24 mu m sources, the inferred CIB lies within 1.1 sigma and 0.5 sigma from direct measurements in the two bands, and fractions increase to 50% and 75%. Most of this resolved CIB fraction was radiated at z <= 1.0, with 160 mu m sources found at higher redshift than 100 mu m ones.

• 出版日期2010-8
• 单位中国地震局