ISO deep far-infrared survey in the Lockman Hole

Details ISO deep far-infrared survey in the Lockman Hole ISO deep far-infrared survey in the Lockman Hole

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427.1017k&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 1017

Physics

3

Galaxies, Evolution, Formation, Quasars, General, Starburst, Cosmology, Observations, Infrared

Scientific paper

Two 44 arcmin x 44 arcmin fields in the Lockman Hole were mapped at 95 and 175 μm using ISOPHOT. A simple program code combined with PIA works well to correct for the drift in the detector responsivity. The number density of 175 μm sources is 3 - 10 times higher than expected from the no-evolution model. The source counts at 95 and 175 μm are consistent with the cosmic infrared background.

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