GOODS J123624.30+621017.3 , the SIMBAD biblio

GOODS J123624.30+621017.3 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:47:43


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Title First 3 Authors
1999ApJ...526L..73R 35 84 Optically faint microjansky radio sources. RICHARDS E.A., FOMALONT E.B., KELLERMANN K.I., et al.
2000AJ....119..292B 41 57 HST/WFPC2 and VLT/ISAAC observations of proplyds in the giant H II region NGC 3603. BRANDNER W., GREBEL E.K., CHU Y.-H., et al.
2000AJ....119.2092B 94 278 Mapping the evolution of high-redshift dusty galaxies with submillimeter observations of a radio-selected sample. BARGER A.J., COWIE L.L. and RICHARDS E.A.
2000ApJ...533..611R viz 14       D               386 259 The nature of radio emission from distant galaxies: the 1.4 GHz observations. RICHARDS E.A.
2005MNRAS.358.1159M viz 15       D               118 104 High-resolution studies of radio sources in the Hubble Deep and flanking fields. MUXLOW T.W.B., RICHARDS A.M.S., GARRINGTON S.T., et al.
2007ApJ...654..764B 21 45 The microjansky radio galaxy population. BARGER A.J., COWIE L.L. and WANG W.-H.
2010ApJS..188..178M viz 15       D               1 1193 129 Very Large Array 1.4 GHz observations of the GOODS-North field: data reduction and analysis. MORRISON G.E., OWEN F.N., DICKINSON M., et al.
2011A&A...533A.119E viz 15       D               1 3965 926 GOODS-Herschel: an infrared main sequence for star-forming galaxies. ELBAZ D., DICKINSON M., HWANG H.S., et al.
2014ApJ...784....9B viz 15       D               1 60 82 Is there a maximum star formation rate in high-redshift galaxies? BARGER A.J., COWIE L.L., CHEN C.-C., et al.
2014ApJS..214...24S viz 15       D               1 97940 733 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al.
2017ApJ...837..139C viz 16       D               1 130 52 A SUbmillimeter PERspective on the GOODS fields (SUPER GOODS). I. An ultradeep SCUBA-2 survey of the GOODS-N. COWIE L.L., BARGER A.J., HSU L.-Y., et al.

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