[SWM2014] GOODS-S 672 , the SIMBAD biblio

[SWM2014] GOODS-S 672 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST17:25:46


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Title First 3 Authors
2004ApJ...600L..93G viz 15       D               1 7819 1453 The Great Observatories Origins Deep Survey: initial results from optical and near-infrared imaging. GIAVALISCO M., FERGUSON H.C., KOEKEMOER A.M., et al.
2008ApJS..179...19L viz 15       D               1 586 273 The Chandra Deep Field-South survey: 2 Ms source catalogs. LUO B., BAUER F.E., BRANDT W.N., et al.
2010ApJS..187..560L viz 15       D               1 469 134 Identifications and photometric redshifts of the 2 Ms Chandra Deep Field-South sources. LUO B., BRANDT W.N., XUE Y.Q., et al.
2011ApJS..195...10X viz 15       D               1 782 508 The Chandra Deep Field-South survey: 4 Ms source catalogs. XUE Y.Q., LUO B., BRANDT W.N., 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.
2014ApJ...796...60H viz 15       D               1 1489 120 CANDELS/GOODS-S, CDFS, and ECDFS : photometric redshifts for normal and X-Ray-detected galaxies. HSU L.-T., SALVATO M., NANDRA K., 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.
2016ApJ...830...51S viz 16       D               1 67525 168 The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al.
2018MNRAS.475.5133R viz 16       D               1 11242 2 Testing the hierarchical assembly of massive galaxies using accurate merger rates out to z ∼ 1.5. RODRIGUES M., PUECH M., FLORES H., et al.

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