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Final analysis of ELAIS 15-$mu$m (Vaccari+, 2005)

Vaccari, M.; Lari, C.; Angeretti, L.; Fadda, D.; Gruppioni, C.; Pozzi, F.; Prouton, O.; Aussel, H.; Babbedge, T.; Ciliegi, P.; Franceschini, A.; Gonzalez-Solares, E.; Franca, F.L.; Oliver, S.; Perez-Fournon, I.; Rowan-Robinson, M.; Serjeant, S. and Vaisanen, P. (2005). Final analysis of ELAIS 15-$mu$m (Vaccari+, 2005). Not Set.

URL: http://vizier.cfa.harvard.edu/viz-bin/VizieR?-sour...
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Abstract

We present the final analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 15-{mu}m observations, carried out with the ISO Camera (ISOCAM) instrument on board the ISO.
The data-reduction method, known as the Lari Method, is based on a mathematical model of the behaviour of the detector and was specifically designed for the detection of faint sources in ISOCAM/ISO Photopolarimeter (ISOPHOT) data. The method is fully interactive and leads to very reliable and complete source lists.
The resulting catalogue includes 1923 sources detected with signal-to-noise ratio of >5 in the 0.5-100mJy flux range and over an area of 10.85deg2 split into four fields, making it the largest non-serendipitous extragalactic source catalogue obtained to date from the ISO data.
(1 data file).

Item Type: Other
Keywords: 15umfa.dat; 1923x156 Whole; 15{mu}m Final Analysis Catalogue
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 5641
Depositing User: Users 13 not found.
Date Deposited: 24 Oct 2006
Last Modified: 02 Dec 2010 19:54
URI: http://oro.open.ac.uk/id/eprint/5641
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