GOODS J123701.53+622024.8 , the SIMBAD biblio

GOODS J123701.53+622024.8 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST02:49:28


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Title First 3 Authors
2000ApJ...533..611R viz 14       D               386 259 The nature of radio emission from distant galaxies: the 1.4 GHz observations. RICHARDS E.A.
2009ApJ...694.1517D 92       D S             2 65 309 Two bright submillimeter galaxies in a z = 4.05 protocluster in GOODS-North, and accurate radio-infrared photometric redshifts. DADDI E., DANNERBAUER H., STERN D., et al.
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.
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.
2016ApJS..222....4S 16       D               1 75 12 Identification of z ≳ 2 Herschel 500 µM sources using color deconfusion. SHU X.W., ELBAZ D., BOURNE N., et al.
2016ApJS..225...27M viz 16       D               1 19341 548 The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ∼ 100,000 galaxies. MOMCHEVA I.G., BRAMMER G.B., VAN DOKKUM P.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.
2018ApJS..235...34O viz 16       D               1 799 10 Deep JVLA imaging of GOODS-N at 20 cm. OWEN F.N.
2024A&A...689A.327W viz 18       D               1 211 ~ The fundamental plane of black hole activity for low-luminosity radio active galactic nuclei across 0 < z < 4. WANG Y., WANG T., HO L.C., et al.

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