A far infrared view of the Lockman Hole from ISO 95 $μ$m observations - I. A new data reduction method

Details A far infrared view of the Lockman Hole from ISO 95 $μ$m observations - I. A new data reduction method A far infrared view of the Lockman Hole from ISO 95 $μ$m observations - I. A new data reduction method

2003-04-14

arxiv.org/abs/astro-ph/0304247v1

Mon.Not.Roy.Astron.Soc. 343 (2003) 1155

Astronomy and Astrophysics

Astrophysics

37 pages, LaTeX file (mn style), 15 figures. Accepted for publication in MNRAS

Scientific paper

10.1046/j.1365-8711.2003.06730.x

We report results of a new analysis of a deep 95 mu imaging survey with the photo-polarimeter ISOPHOT on board the Infrared Space Observatory, over a half square degree area within the Lockman Hole. To this end we exploit a newly developed parametric algorithm able to identify and clean spurious signals induced by cosmic-rays impacts and by transient effects and non-linearities in the detectors. These results provide us with the currently deepest -- to our knowledge -- far-IR image of the extragalactic sky. Within the survey area we detect thirty-six sources with S/N>3 (corresponding to a flux of 16 mJy), making up a complete flux-limited sample around 100$ mJy. Reliable sources are detected, with decreasing but well-controlled completeness, down to 20 mJy. The source extraction process and the completeness, the photometric and astrometric accuracies of this catalogue have been tested by us with extensive simulations accounting for all the details of the procedure. We estimate source counts down to a flux of ~30 mJy, at which limit we evaluate that from 10% to 20% of the cosmic IR background has been resolved into sources. The 95mu galaxy counts reveal a steep slope at fluxes lower than 100 mJy (alpha~1.6), in excess of that expected for a non-evolving source population. The shape of these counts agrees with those determined by ISO at 15 and 175 mu, and starts setting strong constraints on the evolution models for the far-IR galaxy populations.

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