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Journal Paper

전체
The Herschel-PACS North Ecliptic Pole Survey SCI
  • Chris PEARSON;Laia BARRUFET;Maria del Carmen CAMPOS VARILLAS;Stephen SERJEANT;David L. CLEMENTS;Tomotsugu GOTO;Myungshin IM;Jeong Woong-Seob;Seong Jin KIM;Hideo MATSUHARA;Chris SEDGWICK;Ivan VALTCHANOV
  • 2019-01-01
  • PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 71 1 : 13-1~13-11
A detailed analysis of Herschel/Photoconductor Array Camera and Spectrometer (PACS) observations at the North Ecliptic Pole is presented. High-quality maps, covering an area of 0.44?deg2, are produced and then used to derive potential candidate source lists. A rigorous quality-control pipeline has been used to create final legacy catalogues in the PACS Green 100?μm and Red 160?μm bands, containing 1384 and 630 sources respectively. These catalogues reach to more than twice the depth of the current archival Herschel/PACS Point Source Catalogue, detecting 400 and 270 more sources in the short- and long-wavelength bands, respectively. Galaxy source counts are constructed that extend down to flux densities of 6?mJy and 19?mJy (50% completeness) in the Green 100?μm and Red 160?μm bands, respectively. These source counts are consistent with previously published PACS number counts in other fields across the sky. The source counts are then compared with a galaxy evolution model which identifies a population of luminous infrared galaxies as responsible for the bulk of the galaxy evolution over the flux range (5?100?mJy) spanned by the observed counts, contributing approximate fractions of 50% and 60% to the cosmic infrared background at 100?μm and 160?μm, respectively.