GEMS J033236.16-273955.7 , the SIMBAD biblio

GEMS J033236.16-273955.7 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.17CEST00:43:19


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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.
2008AJ....135.1207M 26 28 Triggered or self-regulated star formation within intermediate redshift luminous infrared galaxies. I. Morphologies and spectral energy distributions. MELBOURNE J., AMMONS M., WRIGHT S.A., et al.
2008ApJ...684.1026A viz 15       D               1 509 28 Cosmic evolution of stellar disk truncations: from z∼1 to the Local Universe. AZZOLLINI R., TRUJILLO I. and BECKMAN J.E.
2010A&A...512A..12B viz 15       D               1 4352 228 The Great Observatories Origins Deep Survey. VLT/VIMOS spectroscopy in the GOODS-South field: part II. BALESTRA I., MAINIERI V., POPESSO P., 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.
2011ApJ...743..146C viz 15       D               1 4132 61 Active and passive galaxies at z ∼ 2: rest-frame optical morphologies with WFC3. CAMERON E., CAROLLO C.M., OESCH P.A., et al.
2012MNRAS.425.2116C viz 15       D               2 7382 55 The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS spectroscopic survey of the Chandra Deep Field-South. COOPER M.C., YAN R., DICKINSON M., et al.
2016ApJ...830...51S viz 16       D               1 67524 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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