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

Details Final analysis of ELAIS 15-{mu}m (Vaccari+, 2005) Final analysis of ELAIS 15-{mu}m (Vaccari+, 2005)

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ycat..73580397v&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/358/397. Originally published in: 2005MNRAS.358..397V

Mathematics

Surveys, Galaxies: Ir

Scientific paper

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).

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