The Radio/Optical Catalog of the SSA 13 Field
Author(s) -
E. B. Fomalont,
K. I. Kellermann,
L. L. Cowie,
P. Capak,
A. J. Barger,
R. B. Partridge,
Rogier A. Windhorst,
E. A. Richards
Publication year - 2006
Publication title -
the astrophysical journal supplement series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.546
H-Index - 277
eISSN - 1538-4365
pISSN - 0067-0049
DOI - 10.1086/508169
Subject(s) - physics , astrophysics , hubble deep field , galaxy , subaru telescope , radio galaxy , source counts , astronomy , redshift , brightness , spectral index , hubble deep field south , spectrograph , spectral line
We present a 1.4-GHz catalog of 810 radio sources (560 sources in thecomplete sample) with 1.8" resolution found within a 17' radius in the SSA13field (RA=13h12m,DEC=42d38'). The radio image from the VLA has an rms noiselevel of 4.82 microJy/beam at the field center, and Subaru optical images inr-band (6300A) and z-band (9200A) have a three-sigma detection magnitude of26.1 and 24.9, respectively. 88% of the radio sources are identified with anoptical counterpart, and there is significantly more reddening for objectsfainter than 24-mag. The radio and optical parameters are tabulated, and sourcemorphologies are displayed by radio contours overlaying optical false-colorimages. The radio structures show a wealth of complexity and these areclassified into a small number of categories. About one-third of the radiosources are larger than 1.2" and their orientation is often similar to that ofthe associated galaxy or binary-galaxy system. The density of sources in theSSA13 field above 75 microJy is 0.40 per square arcmin, with a slope of -2.43in the differential counts. The radio spectral index may steepen for sourcesbelow 75 microJy. We estimate that at most 40% of the microJansky radio sourcesare dominated by AGN processes.Comment: 50 pages, 14 figures of which fig 6 contains 33 parts. In press, Astrophysical Journal, Supp
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