RADIO-EMISSION FROM GALAXIES IN THE HUBBLE DEEP FIELD

We report on sensitive radio observations made with the VLA at 8.5 GHz centered on the Hubble Deep Field (HDF). We collected data in the A, CnB, C, DnC, and D configurations corresponding to angular resolutions ranging from 0.'' 3 to 10 ''. We detected 29 radio sources in a compl ete sample within 4.'6 of the HDF center and above a flux density limi t of 9.0 mu Jy (5 sigma). Seven of these sources are located within th e HDF itself, while the remaining 22 sources are covered by the Hubble flanking fields (HFFs) or ground-based optical images. All of the sou rces in the HDF are identified with galaxies with a mean magnitude R = 21.7, while the mean magnitude of the identifications outside the HDF is R = 22.1. One radio source in the HDF, which is just below our for mal completeness level but is confirmed by independent 1.4 GHz observa tions, has no optical counterpart above the HDF limit of R = 29. Three radio sources outside the HDF have no optical counterparts to R = 27. Based on a radio and optical positional coincidence, we detected an a dditional 19 radio sources in this held (seven of which are contained in the HDF) with 6.3 mu Jy less than or equal to S-v < 9.0 mu Jy (3.5 sigma less than or equal to S-v < 5 sigma) and R less than or equal to 25 but which are not included in the complete sample. The microjansky radio sources are distributed over a wide range of redshifts (0.1 < z < 3) and have a typical monochromatic luminosity of about 10(23) W Hz (-1). The majority of the optical identifications are with luminous (L > L) galaxies at modest redshifts (0 less than or similar to z less than or similar to 1), many with evidence for recent star formation. T he remainder are composed of a mixture of bright held elliptical galax ies and late-type galaxies with evidence of nuclear activity (LINERs a nd Seyfert galaxies) and nearby (z < 0.2) held spiral galaxies. None o f the radio sources in this survey are identified with quasars or gala ctic stars.