A&A 475, 791-799 (2007)
DOI: 10.1051/0004-6361:20065218
A 12
m ISOCAM survey of the ESO-Sculptor field
Data reduction and analysis
N. Seymour1, 2, B. Rocca-Volmerange1, 3, and V. de Lapparent11 Institut d'Astrophysique de Paris, UMR7095 CNRS / Univ. Pierre & Marie Curie, 98 bis boulevard Arago, 75014 Paris, France
e-mail: seymour@ipac.caltech.edu
2 Science Center, California Institute of Technology, Mail Code 220-6, 1200 East California Boulevard, Pasadena, CA 91125, USA
3 Université Paris-Sud, Bât. 121, 91405 Orsay Cedex, France
(Received 16 March 2006 / Accepted 24 May 2007 )
Abstract
We present a detailed reduction of a mid-infrared 12
m (LW10 filter)
ISOCAM open time observation performed on the ESO-Sculptor Survey field
(Arnouts et al. 1997, A&AS, 124, 163). A complete catalogue of 142 sources (120 galaxies and
22 stars), detected with high significance (equivalent to 5
),
is presented above an integrated flux density of 0.24
. Star/galaxy
separation is performed by a detailed study of colour-colour diagrams.
The catalogue is complete
to 1
and, below this flux density, the incompleteness is corrected
using two independent methods. The first method uses stars and the second
uses optical counterparts of the ISOCAM galaxies;
these methods yield consistent results. We also apply
an empirical flux density calibration using stars in the field. For each
star, the 12
m flux density is derived by fitting optical colours
from a multi-band
to stellar templates (BaSel-2.0) and using empirical optical-IR
colour-colour relations. This article is
a companion analysis to our 2007 paper (Rocca-Volmerange et al. 2007, A&A, 475, 801) where the
faint galaxy
counts are presented and analysed per galaxy type with the evolutionary code PÉGASE.3.
Key words: infrared: galaxies -- Galaxy: evolution -- methods: data analysis -- catalogs -- galaxies: photometry
© ESO 2007

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