English

Optically Faint Microjansky Radio Sources

Astrophysics 2009-10-31 v1

Abstract

We report on the identifications of radio sources from our survey of the Hubble Deep Field and the SSA13 fields, both of which comprise the deepest radio surveys to date at 1.4 GHz and 8.5 GHz respectively. About 80% of the microjansky radio sources are associated with moderate redshift starburst galaxies or AGNs within the I magnitude range of 17 to 24 with a median of I = 22 mag. Thirty-one (20%) of the radio sources are: 1) fainter than I>I>25 mag, with two objects in the HDF IAB>I_{AB}>28.5, 2) often identified with very red objects IK>I-K>4, and 3) not significantly different in radio properties than the brighter objects. We suggest that most of these objects are associated with heavily obscured starburst galaxies with redshifts between 1 and 3. However, other mechanisms are discussed and cannot be ruled out with the present observations.

Keywords

Cite

@article{arxiv.astro-ph/9909251,
  title  = {Optically Faint Microjansky Radio Sources},
  author = {E. A. Richards and E. B. Fomalont and K. I. Kellermann and R. A. Windhorst and R. B Partridge and L. L. Cowie and A. J. Barger},
  journal= {arXiv preprint arXiv:astro-ph/9909251},
  year   = {2009}
}

Comments

to appear in Astrophysical Journal Letters, 3 figures, 1 table

R2 v1 2026-07-22T09:51:12.797Z