A catalog for the north and south Galactic caps
(811,117 sources), derived from the
1993 through 2002 observations, is
currently available as a gzip-compressed ASCII file
The file size is 26.6 Mbytes compressed (87.6 Mbytes uncompressed).
The catalog covers a total of about 9033 square degrees of sky (8422
square degrees in the north Galactic cap and 611 square degrees
in the south Galactic cap.)
See the coverage maps for more details of the area covered. Both the northern and southern areas were chosen to concide the area planned to be covered by the Sloan Digital Sky Survey. No new sky area was covered in the south Galactic cap during the past observing season, although the southern equatorial strip was reobserved. The results of the repeated observations will be released separately; the current catalog is identical to the previous catalog in the south.
The catalog is on-line and can be searched using the FIRST Search Engine. However, for large-scale investigations it will be necessary to obtain the complete catalog. This document describes the catalog format.
The catalog is sorted by right ascension and has the following format:
RA (2000) Dec W Fpeak Fint Rms Maj Min PA fMaj fMin fPA Field Name 06 50 44.043 +31 10 00.09 1.16 0.64 0.147 0.00 0.00 42.0 4.50 3.59 42.0 06510+31143E 06 51 02.181 +31 11 13.33 1.58 2.66 0.139 4.99 3.94 91.6 7.35 6.69 91.6 06510+31143E 06 51 03.826 +31 13 03.32 W 1.02 1.42 0.137 7.63 0.00 2.4 9.35 4.34 2.4 06510+31143E 06 51 06.134 +31 19 02.00 7.29 9.64 0.145 4.09 1.82 131.3 6.77 5.70 131.3 06510+31143E 06 51 10.784 +31 11 28.80 72.36 100.79 0.141 4.18 2.49 9.8 6.83 5.95 9.8 06510+31143ENote that this format is the same as in all versions of the catalog released since 1997; older versions have a different format.
unc(90% confidence) = Size (1/SNR + 1/20) arcsecwhere Size is either the major or minor axis fitted FWHM (fMaj or fMin) as given in the catalog and SNR is the peak flux density signal-to-noise ratio:
SNR = (Fpeak-0.25) / Rms(The positional uncertainty is of course elliptical for elliptical sources.) The best possible positional uncertainty is limited to about 0.1 arcsec by our ability to fit source positions in maps with 1.8 arcsec pixels and by various random calibration uncertainties. Systematic errors in the positions are smaller than 0.05 arcsec.
IMPORTANT NOTE: The sidelobe flagging near and south of the equator is not as reliable as in the north because the sidelobe characteristics change with the zenith angle of the observation. We are working on improvements to the sidelobe-flagging, but for now it is important to be cautious in studies of individual southern sources. We recommend checking the images using the FIRST Cutout Server if there is any doubt about the reality of particular sources (in either the north or the south.) This is easily done when using the FIRST Search Engine to search the catalog, since each source selected in the search has a link to the Cutout Server.
The uncertainty in Fpeak is given by the rms noise at the source position, while the uncertainty in Fint can be considerably greater depending on the source size and morphology. For bright sources the accuracies of Fpeak and Fint are limited to about 5% by systematic effects. Note that for sources that are not well-described by an elliptical Gaussian model, Fint is not an accurate measure of the integrated flux density.
FITS images giving the rms noise as a function of position on the sky are available for the northern and the southern areas. These images give the rms in mJy/beam tabulated on a ~3 arcmin grid in RA and Declination. If there is no source in the catalog at a given position, the source peak flux density (before CLEAN bias correction) is less than 5 times the coverage map rms value at that position. The sky area covered is displayed in the images below (which are linked to postscript versions of the images):
Noise can cause the fitted values of the major and minor axes (before deconvolution) to be smaller than the beam. The corresponding deconvolved size is given as zero in those cases.
The uncertainties in the deconvolved sizes depend on both the brightness and the sizes. Objects at the catalog flux density limit have uncertainties of about 2 arcsec in their sizes (so faint objects with Maj < 2 arcsec are consistent with point sources.) An simple empirical estimate of the uncertainty is
Sigma(Size) = 10 arcsec (1/SNR + 1/75)where SNR is the signal-to-noise ratio defined above.
hhmmm+ddmmmis centered at RA=
hh mm.m, Dec=
+dd mm.m. The images are available from several archives and through the FIRST Cutout Server.
All field names in the current catalog end with a letter E through J, depending on the date of the last catalog release in which the image was modified. The J fields are new in this catalog, while sources extracted from the E/F/G/H/I fields are nearly identical to those in the previous version of the catalog.
The catalog history page describes previously released versions of the FIRST catalogs, which are still available for historical purposes. We recommend that the new catalog be used where possible for all projects.