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-m (Vaccari+, 2005).
URL: | http://vizier.cfa.harvard.edu/viz-bin/VizieR?-sour... |
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Dataset Google Scholar: | Look up in Google Scholar |
Abstract
We present the final analysis of the European Large Area Infrared Space Observatory (ISO) Survey (ELAIS) 15-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: | Research Dataset Record |
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Dataset Status: | Finalised |
Dataset Access: | http://vizier.cfa.harvard.edu/viz-bin/VizieR?-source=J/MNRAS/358/397 |
Retention Rule: | Indefinitely |
Retention Action: | Archive |
Keywords: | 15umfa.dat; 1923x156 Whole; 15{mu}m Final Analysis Catalogue |
Academic Unit or School: | Physical Sciences Faculty of Science, Technology, Engineering and Mathematics (STEM) |
Item ORO ID: | 5641 |
Depositing User: | ORO Import |
Date Deposited: | 24 Oct 2006 |
Last Modified: | 22 May 2024 04:30 |
URI: | https://oro.open.ac.uk/id/eprint/5641 |