The Astrophysical Journal Supplement Series · 2006 · 75 citations · 24 references
Natural SciencesAstronomyPhysicsExtragalactic AstronomyObservational AstronomyRadio AstronomyExtragalactic Radio AstronomyRadio TelescopesSpace-based Gamma-ray ObservatoriesExtragalactic Radio SourcesRadio Source MorphologyRadio SurveysSpectral Brightness
We present a 1.4-GHz catalog of 810 radio sources (560 sources in the complete sample) with 1.8" resolution found within a 17' radius in the SSA13 field (RA=13h12m,DEC=42d38'). The radio image from the VLA has an rms noise level of 4.82 microJy/beam at the field center, and Subaru optical images in r-band (6300A) and z-band (9200A) have a three-sigma detection magnitude of 26.1 and 24.9, respectively. 88% of the radio sources are identified with an optical counterpart, and there is significantly more reddening for objects fainter than 24-mag. The radio and optical parameters are tabulated, and source morphologies are displayed by radio contours overlaying optical false-color images. The radio structures show a wealth of complexity and these are classified into a small number of categories. About one-third of the radio sources are larger than 1.2" and their orientation is often similar to that of the associated galaxy or binary-galaxy system. The density of sources in the SSA13 field above 75 microJy is 0.40 per square arcmin, with a slope of -2.43 in the differential counts. The radio spectral index may steepen for sources below 75 microJy. We estimate that at most 40% of the microJansky radio sources are dominated by AGN processes.
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The International Celestial Reference Frame as Realized by Very Long Baseline Interferometry
Chao Ma, E. F. Arias, T. M. Eubanks et al. · The Astronomical Journal · 1998 · 775 citations · Full text
Natural Sciences, Astronomy, Physics +14
The VLBA Calibrator Survey—VCS1
The Astrophysical Journal Supplement Series · 2002 · 333 citations · Full text
Natural Sciences, Astronomy, Physics +17