ACO 370, 2218 and 2390 fluxes at 7 and 15um (Metcalfe+, 2003)

Details ACO 370, 2218 and 2390 fluxes at 7 and 15um (Metcalfe+, 2003) ACO 370, 2218 and 2390 fluxes at 7 and 15um (Metcalfe+, 2003)

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..34070791m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/407/791. Originally published in: 2003A&A...407..791M

Physics

Clusters: Galaxy, Infrared Sources

Scientific paper

ESA's Infrared Space Observatory (ISO) was used to perform a deep survey with ISOCAM through three massive gravitationally lensing clusters of galaxies. The total area surveyed depends on source flux, with nearly seventy square arcminutes covered for the brighter flux levels in maps centred on the three clusters Abell 370, Abell 2218 and Abell 2390. We present maps and photometry at 6.7um (hereafter 7um) and 14.3um (hereafter 15um), showing a total of 145 mid-infrared sources and the associated source counts.
(6 data files).

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