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A&A 419, L55-L58 (2004)
DOI: 10.1051/0004-6361:20040144
Letter
ISOPHOT 95
m observations in the Lockman Hole
The catalogue and an assessment of the source counts
G. Rodighiero and A. FranceschiniDipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35122 Padova, Italy
(Received 16 March 2004 / Accepted 15 April 2004)
Abstract
We report results from a new analysis of a deep 95
m imaging
survey with ISOPHOT on board the Infrared Space Observatory, over a ~1 deg
2 area within the Lockman Hole, which extends the statistics
of our previous study (Rodighiero et al. 2003).
Within the survey area we detect sixty-four sources with
(roughly
corresponding to a flux limit of 16 mJy). Extensive simulations indicate that
the sample is almost complete at
mJy, while the
incompleteness can be quantified down to ~30 mJy.
The 95
m galaxy counts reveal a steep slope at
mJy (
), in excess of that expected for a non-evolving source
population. In agreement with counts data from ISO at 15 and 175
m,
this favours a model where the IR populations evolve both
in number and luminosity densities. We finally comment on some differences
found with other ISO results in this area.
Key words: infrared: galaxies -- galaxies: photometry, statistics, evolution
Offprint request: G. Rodighiero, rodighiero@pd.astro.it
SIMBAD Objects
© ESO 2004
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