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The European Large Area ISO Survey - VIII. 90-μm final analysis and source counts

Héraudeau, Ph.; Oliver, S.; del Burgo, C.; Kiss, C.; Stickel, M.; Mueller, T.; Rowan-Robinson, M.; Efstathiou, A.; Surace, C.; Tóth, L.V.; Serjeant, S. and Alexander, D.M. [et al.] (2004). The European Large Area ISO Survey - VIII. 90-μm final analysis and source counts. Monthly Notices of the Royal Astronomical Society, 354(4) pp. 961–970.

URL: http://arxiv.org/abs/astro-ph/0408045
DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1111/j.1365-2966.2004.08259.x
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Abstract

This paper discusses the properties of the European Large Area ISO Survey (ELAIS) 15-μm quasars and tries to establish a robust method of quasar selection for future use within the Spitzer Wide-Area Infrared Extragalactic Survey (SWIRE) framework. The importance of good-quality ground-based optical data is stressed, both for the selection of candidates and for the estimation of photometric redshifts. Colour-colour plots and template fitting are used for these purposes. The properties of the 15-μm quasar sample, including variability and black hole masses, are studied and compared to the properties of other quasars that lie within the same fields but have no mid-infrared counterparts. The two subsamples do not present substantial differences and are believed to come from the same parent population.

Item Type: Journal Article
Copyright Holders: 2004 RAS, MNRAS
ISSN: 1365-2966
Keywords: surveys; galaxies; evolution; formation; infrared
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 5662
Depositing User: Users 13 not found.
Date Deposited: 25 Oct 2006
Last Modified: 11 Jul 2013 15:25
URI: http://oro.open.ac.uk/id/eprint/5662
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