  The Very Large Array (VLA) has been used in C-configuration to map an area
\~0.3 square degrees at 1.4 GHz with 5sigma sensitivities of 0.305, 0.325,
0.380 and 0.450 mJy/beam over four equal subareas. Radio properties are
presented for 62 detected sources. Deep optical imaging to Gunn r~25 mag using
the Hale 5-m telescope covering ~0.21 square degrees is reported for a subset
of 43 sources. This optical follow-up is much deeper than that of existing
larger area radio surveys of similar radio sensitivity. Archival J, H and
K-band photometry from the Two-Micron All Sky Survey (2MASS) is also presented.
Using a robust likelihood-ratio technique, we optically identified 26 radio
sources with probabilities >80%. Nine are uncertain/ambiguous detections and
eight are empty fields. Comparisons with a stellar synthesis model that
includes radio emission and dust reddening suggests that the
near-infrared--to--optical emission in a small, bright sub-sample is reddened
by `optically-thin' dust with absorption A_V ~ 2-2.5 mag, regardless of
morphological type. This is consistent with other, more direct determinations
of absorption. The radio--to--optical(--near-infrared) flux ratios of
early-type galaxies require significant contamination in the radio by an active
galactic nucleus (AGN), consistent with the current paradigm. Using our simple
modeling approach, we also discuss a potential diagnostic for selecting
Ultraluminous Infrared Galaxies (ULIGS) to z~1.6 from microJansky radio
surveys.
