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2005MNRAS.358..397V - Mon. Not. R. Astron. Soc., 358, 397-418 (2005/April-1)
Final analysis of ELAIS 15-µm observations: method, reduction and catalogue.
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.
Abstract (from CDS):
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.
This paper presents the concepts underlying the data-reduction method together with its latest enhancements. The data-reduction process, the production and basic properties of the resulting catalogue are discussed. The catalogue quality is assessed by means of detailed simulations, optical identifications and comparison with previous analyses.
Abstract Copyright: 2005 RAS
Journal keyword(s): methods: data analysis - catalogues - galaxies: active - galaxies: evolution - galaxies: formation - infrared: galaxies
VizieR on-line data: <Available at CDS (J/MNRAS/358/397): 15umfa.dat>
Status at CDS : All or part of tables of objects could be ingested in SIMBAD with priority 2.
Simbad objects: 7
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