Richard G. McMahon
University of Cambridge, Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, England
Richard L. White
Space Telescope Science Institute, 3700 San Martin Dr., Baltimore, MD 21218
David J. Helfand
Astronomy Dept., Columbia University, New York, NY 10027
Robert H. Becker
Physics Dept., University of California, Davis, CA 95616
and IGPP/Lawrence Livermore National Laboratory
We describe a program to identify optical counterparts to radio
sources from the VLA FIRST survey using the Cambridge APM
scans of the POSS-I plates. We use radio observations covering 4150
deg of the north Galactic cap to a 20 cm flux density threshold
of 1.0 mJy; the 382,892 sources detected all have positional
uncertainties of
(radius of 90% confidence).
Our description of the APM catalog, derived from the 148 POSS-I
and
plates covering this region, includes an assessment of its
astrometric and photometric accuracy, a photometric recalibration
using the Minnesota APS catalog, a discussion of the classification
algorithm, and quantitative tests of the catalog's reliability and
completeness. We go on to show how the use of FIRST sources as
astrometric standards allows us to improve the absolute astrometry
of the POSS plates by nearly an order of magnitude to
rms. Matching the radio and optical catalogs
yields counterparts for over 70,000 radio sources; we include
detailed discussions of the reliability and completeness of these
identifications as a function of optical and radio morphology,
optical magnitude and color, and radio flux density. An analysis of
the problem of radio sources with complex morphologies (e.g.,
double-lobed radio galaxies) is included. We conclude with a brief
discussion of the source classes represented among the radio sources
with identified counterparts.
Keywords: surveys - catalogs - quasars:general - galaxies:general - radio continuum:general