Optically faint microjansky radio sources

被引:84
作者
Richards, EA
Fomalont, EB
Kellermann, KI
Windhorst, RA
Partridge, RB
Cowie, LL
Barger, AJ
机构
[1] Natl Radio Astron Observ, Charlottesville, VA 22903 USA
[2] Univ Virginia, Dept Phys & Astron, Charlottesville, VA 22903 USA
[3] Haverford Coll, Dept Phys & Astron, Haverford, PA 19041 USA
[4] Univ Hawaii, Honolulu, HI 96822 USA
关键词
galaxies : evolution; galaxies : starburst; radio continuum : general;
D O I
10.1086/312373
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the identifications of radio sources from our survey of the Hubble Deep Field (HDF) and the Small Selected Area 13 fields, both of which comprise the deepest radio surveys to date at 1.4 and 8.5 GHz, respectively. About 80% of the microjansky radio sources are associated with moderate-redshift starburst galaxies or active galactic nuclei within the I-magnitude range of 17-24 with a median of I = 22 mag. Thirty-one (20%) of the radio sources are (1) fainter than I > 25 mag, with two objects in the HDF I-AB > 28.5, (2) often identified with very red objects 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.
引用
收藏
页码:L73 / L76
页数:4
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