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dc.contributor.authorYan, Haojingen_US
dc.contributor.authorWindhorst, Rogier A.en_US
dc.contributor.authorRottgering, Huub J. A.en_US
dc.contributor.authorCohen, Seth H.en_US
dc.contributor.authorOdewahn, Stephen C.en_US
dc.contributor.authorChapman, Scott C.en_US
dc.contributor.authorKeel, William C.en_US
dc.date.accessioned2014-03-12T19:21:04Z
dc.date.available2014-03-12T19:21:04Z
dc.date.issued2003-03en_US
dc.identifier.citationYan, Haojing, Rogier A. Windhorst, Huub J. A. Rottgering, Seth H. Cohen, et al. 2003. "The Infrared Counterparts of the Optically Unidentified CDF-S 1Ms Sources." The Astrophysical Journal 585(1): 67-72en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://dx.doi.org/10.1086/345998en_US
dc.identifier.urihttp://hdl.handle.net/10222/45471
dc.description.abstractThe Chandra Deep Field South (CDF-S) 1Ms exposure produced a catalog of 346 X-ray sources, of which 59 were not visible on the VLT/FORS1 and the ESO-MPI/WFI deep R-band images to a limit of R_{vega}=26.1--26.7 mag. Using the first release of the ESO VLT/ISAAC JHK_s data on the CDF-S, we identified six of the twelve such objects that were within the coverage of these IR observations. The VLT/FORS1 I-band data further confirms that five of these six objects are undetected in the optical. The photometric properties of these six counterparts are compared against those of the optically brighter counterparts of Chandra sources in the same field. We found that the location of these optically brighter Chandra sources in the near-IR color space was bifurcated, with the color of one branch being consistent with that of E/S0 galaxies at 0 5) star-forming galaxies nor irregular galaxies at lower redshift can be a viable explanation to the nature of these six counterparts.en_US
dc.titleThe Infrared Counterparts of the Optically Unidentified CDF-S 1Ms Sourcesen_US
dc.title.alternativeThe Astrophysical Journalen_US
dc.typearticleen_US
dc.identifier.volume585en_US
dc.identifier.issue1en_US
dc.identifier.startpage67en_US
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