XMM-LSS field optical identifications (Tasse+, 2008)

Details XMM-LSS field optical identifications (Tasse+, 2008) XMM-LSS field optical identifications (Tasse+, 2008)

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ycat..34900879t&link_type=abstract

VizieR On-line Data Catalog: J/A+A/490/879. Originally published in: 2008A&A...490..879T

Physics

Radio Sources, Cross Identifications, Photometry: Sdss, Photometry: Millimetric/Submm

Scientific paper

We use the radio data described in detail in Tasse et al. (2006, Cat. ). The observations were carried out using the Very Large Array (VLA) at 74 and 325MHz simultaneously (4P mode). The radio survey consists of four pointings, observed in June, July and August 2003 in the A configuration and in June and July 2002 in the B configuration
Low-frequency radio observations of the XMM-LSS have been carried out with the Giant Meterwave Radio Telescope (GMRT) at 230 and 610MHz (Tasse et al., 2007, Cat. ). These data provide two additional flux density measurements for 41% of the radio sources detected at 325MHz with the VLA.
Observations with the CFHTLS-W1 were carried out between June 1, 2003 and Sept. 12, 2005.
Throughout this paper we have used the SWIRE data release 2 band-merged catalog available online (http://swire.ipac.caltech.edu/swire/), containing the flux density measurements at 3.6, 4.5, 5.8, 8.0 and 24um for a total of ~2.5x105^ objects.
(2 data files).

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