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CXOECDFS J033121.5-275704 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST07:26:02 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
---|---|---|---|---|---|---|---|---|---|
2005ApJS..161...21L | 15 | D | 799 | 263 | The Extended Chandra Deep Field-South survey: Chandra point-source catalogs. | LEHMER B.D., BRANDT W.N., ALEXANDER D.M., et al. | |||
2006AJ....131.2373V | 15 | D | 652 | 49 | The Extended Chandra Deep Field-South survey: X-ray point-source catalog. | VIRANI S.N., TREISTER E., URRY C.M., et al. | |||
2008ApJ...680..130C | 15 | D | 1 | 1013 | 61 | Mid-infrared properties and color selection for X-Ray-detected active galactic nuclei in the MUSYC Extended Chandra Deep Field-South. | CARDAMONE C.N., URRY C.M., DAMEN M., et al. | ||
2010ApJS..191..124S | 15 | D | 1 | 781 | 124 | The Extended Chandra Deep Field-South survey: optical spectroscopy of faint X-ray sources with the VLT and Keck. | SILVERMAN J.D., MAINIERI V., SALVATO M., et al. | ||
2012MNRAS.420.2190V | 15 | D | 1 | 124 | 33 | The radio–X-ray relation as a star formation indicator: results from the very large Array–Extended Chandra deep field-south. | VATTAKUNNEL S., TOZZI P., MATTEUCCI F., et al. | ||
2012ApJS..203...15B | 15 | D | 1 | 894 | 38 | The sub-mJy radio population of the E-CDFS: optical and infrared counterpart identification. | BONZINI M., MAINIERI V., PADOVANI P., et al. | ||
2013ApJS..205...13M | 16 | D | 1 | 894 | 109 | The Very Large Array 1.4 GHz survey of the Extended Chandra Deep Field South: second data release. | MILLER N.A., BONZINI M., FOMALONT E.B., et al. | ||
2013MNRAS.436.3759B | 16 | D | 1 | 885 | 125 | The sub-mJy radio sky in the Extended Chandra Deep Field-South: source population. | BONZINI M., PADOVANI P., MAINIERI V., et al. | ||
2015MNRAS.453.1079B | 16 | D | 1 | 781 | 30 | Star formation properties of sub-mJy radio sources. | BONZINI M., MAINIERI V., PADOVANI P., et al. |