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From: Richard L. White
Optical Counterparts for 70,000 Radio Sources: APM Identifications for the
FIRST Radio Survey
Authors:
Richard G. McMahon, Richard L. White, David J. Helfand, Robert H. Becker
Comments: Accepted for publication in ApJ; 28 pages, 23 figures
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 square
degrees 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 <1" (radius of 90% confidence). Our
description of the APM catalog, derived from the 148 POSS-I O and
E 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 ~0.15" 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.
Format for the Table of FIRST-APM Optical Counterparts
From the paper:
Column Name Description
------ ---- -----------
1-2 RA, Dec radio source coordinates (epoch J2000.0)
3-5 dRA, dDec offsets (arcsec) to the optical object in RA and Dec
5 Sep radius (arcsec) to the optical object
6 Ecl APM classification on E plate
7 Epsf APM psf parameter on E plate
8 Emag E (red) magnitude
9 Ocl APM classification on O plate
10 Opsf APM psf parameter on O plate
11 Omag O (blue) magnitude
12 O-E Color
13 Plate Number of POSS-I plate
14 Fpeak FIRST peak radio flux density (mJy)
15 Fint FIRST integrated radio flux density (mJy)
16 Maj FIRST source deconvolved major axis (FWHM, arcsec)
17 Min FIRST source deconvolved minor axis (FWHM, arcsec)
18 PA FIRST position angle for major axis (degrees)
Notes on parameters:
- APM positions and magnitudes have been calibrated as described in the
paper.
- The classification codes (Ecl, Ocl) are -1=stellar, 1=non-stellar,
2=blended, 0=noise.
- The Epsf and Opsf parameters measure by how many sigma the object
deviates from being a point-source.
- Negative magnitudes indicate that source is undetected on the plate.
In that case, the absolute value of the magnitude is an upper limit.
- The O-E color is -9.99 if the object is detected on only one plate.
- The radio parameters are described in more detail in White, Becker,
Helfand, & Gregg (1997, ApJ, 475, 479) and on the FIRST web pages
(http://sundog.stsci.edu).
- Negative values for the FIRST major and minor axes indicate that the
source size before deconvolution was smaller than the beam, so the
source is unresolved along that axis.