A typical coadded FIRST image covering 0.41 contains
pixels,
but only
discrete radio sources above a threshold of 0.75 mJy. Thus,
while the maps are a valuable resource as an archival image of the radio sky,
as well as for such tasks as deriving upper limits to sources
found at other wavelengths, the most useful scientific product of the survey
is the source catalog. Given the highly non-Gaussian characteristics of the
noise in snapshot images and the large variety of morphologies exhibited by
various radio source populations, automatic extraction of a highly reliable
and complete catalog from the FIRST images is a nontrivial task.
However, because of its scientific importance for users, as well as the central
role it plays in characterizing image quality and integrity, we have
expended considerable effort in developing algorithms to produce a source
catalog. We expect to continue these efforts for some time to come.
Nonetheless, we now have a functioning source extraction program which has
generated a preliminary catalog from the 1993 dataset which contains 27,680
entries and
can be retrieved via the FIRST home-page where a more detailed
description can be found.
A paper describing the catalog construction process is in preparation
(White et al. 1995).