| dc.contributor.author | Willner, S. P. | en_US |
| dc.contributor.author | Ashby, M. L. N. | en_US |
| dc.contributor.author | Barmby, P. | en_US |
| dc.contributor.author | Chapman, S. C. | en_US |
| dc.contributor.author | Coil, A. | en_US |
| dc.contributor.author | Cooper, M. | en_US |
| dc.contributor.author | Huang, J. -S | en_US |
| dc.contributor.author | Ivison, R. | en_US |
| dc.contributor.author | Koo, D. C. | en_US |
| dc.date.accessioned | 2014-03-12T19:21:04Z | |
| dc.date.available | 2014-03-12T19:21:04Z | |
| dc.date.issued | 2012-09-01 | en_US |
| dc.identifier.citation | Willner, S. P., M. L. N. Ashby, P. Barmby, S. C. Chapman, et al. 2012. "A Fully-Identified Sample of AEGIS20 Microjansky Radio Sources." 756(1) | en_US |
| dc.identifier.issn | 0004-637X | en_US |
| dc.identifier.uri | http://dx.doi.org/10.1088/0004-637X/756/1/72 | en_US |
| dc.identifier.uri | http://hdl.handle.net/10222/45470 | |
| dc.description.abstract | Infrared 3.6 to 8 micron images of the Extended Groth Strip yield plausible counterpart identifications for all but one of 510 radio sources in the AEGIS20 S(1.4 GHz) > 50 micro-Jy sample. This is the first such deep sample that has been effectively 100% identified. Achieving the same identification rate at R-band would require observations reaching R_AB > 27. Spectroscopic redshifts are available for 46% of the sample and photometric redshifts for an additional 47%. Almost all of the sources with 3.6 micron AB magnitudes brighter than 19 have spectroscopic redshifts z 1 with the remainder of uncertain nature. | en_US |
| dc.title | A Fully-Identified Sample of AEGIS20 Microjansky Radio Sources | en_US |
| dc.title.alternative | The Astrophysical Journal | en_US |
| dc.type | article | en_US |
| dc.identifier.volume | 756 | en_US |
| dc.identifier.issue | 1 | en_US |
| dc.identifier.startpage | | en_US |
