COSMOS VLA Deep Catalog Definitions
COSMOS Overview
The COSMOS Archive serves data taken for the Cosmic Evolution Survey (COSMOS) project. COSMOS is an astronomical survey designed to probe the formation and evolution of galaxies as a function of cosmic time (redshift) and large scale structural environment. The survey covers a 2 square degree equatorial field with imaging by most of the major space-based telescopes (Hubble, Spitzer, GALEX, XMM, Chandra) and a number of large ground based telescopes (Subaru, VLA, ESO-VLT, UKIRT, NOAO, CFHT, and others).
IRSA serves the COSMOS archive using the following search methods:
- Spatial search on all images and small catalogs, using Atlas
- Advanced search on only the larger catalogs, using Gator
COSMOS VLA Deep Catalog
These VLA data represent the additional 62 hrs of 1.4 GHz (20cm) observations of the central 7 pointings already imaged by the large project in A-configuration in February/March 2006. The observations have been combined with the large project in which the 2 square degree COSMOS field with the position given above as the center of the field was surveyed for 275 hours. The observations of the large project were performed at 1.4 GHz (20 cm), using the VLA in its A- and C-configuration between September 2004 and September 2005. The final combined survey has reached a sensitivity of an rms of uJy/beam in the central 30' at a resolution of 2.5"x2.5".The key characteristics of these data:
- Configuration: VLA A-array & C-array
- Dates of observations:
- September, 2004 - January, 2005 (A-array)
- August, 2005 - September, 2005 (C-array)
- February/March, 2006 (A-array: central 7 pointings)
- Observing time:
- 250 hours (A-array)
- 25 hours (C-array)
- 62 hours (A-array: central 7 pointings)
- Frequency: 1.4 GHz ( = L band, 20cm)
- Bandwidth: 75 MHz (Multi-channel continuum mode)
- Pointings: 23 (hexagonal pattern)
- Area: 2 sq degs (box used for source extraction)
- Resolution: 2.5" x 2.5"
- Sensitivity: 10-40 uJy/beam (inner to outermost regions)
The data reduction, image reconstruction, catalog construction and bandwidth correction is similar to the procedures for the large project described in:
"The VLA-COSMOS Survey: II. Source Catalog of the Large Project" by Schinnerer et al. 2007, ApJS, COSMOS special issue, 172, 46
"The VLA-COSMOS Survey: III. Further Catalog Analysis and the Radio Source Counts" by Bondi et al., 2008, ApJ, 681, 1129
More details will be presented by Schinnerer et al. (in prep.) "The VLA-COSMOS Survey: IV. Joint Source Catalog of the Large and Deep Project"
COSMOS VLA Deep Catalog Column Definitions
Gator serves the COSMOS May 2010 VLA Deep Source Catalog (25 columns [20 delivered + 5 IRSA-created], 2,865 data rows). The column descriptions can be found below.