GEMS J033242.56-274550.2 , the SIMBAD biblio

GEMS J033242.56-274550.2 , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST20:48:09

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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
2004A&A...428.1043L viz 15       D               1601 300 The VIMOS VLT Deep Survey. Public release of 1599 redshifts to IAB≤24 across the Chandra Deep Field South. LE FEVRE O., VETTOLANI G., PALTANI S., et al.
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.
2005A&A...434...53V viz 15       D               301 207 The Great Observatories Origins Deep Survey VLT/FORS2 spectroscopy in the GOODS-South Field. VANZELLA E., CRISTIANI S., DICKINSON M., et al.
2005ApJ...623L..71E 37 24 Central blue clumps in elliptical galaxies of the Hubble Ultra Deep Field. ELMEGREEN D.M., ELMEGREEN B.G. and FERGUSON T.E.
2006A&A...449..951G viz 1278 302 The GOODS-MUSIC sample: a multicolour catalog of near-IR selected galaxies in the GOODS-South field. GRAZIAN A., FONTANA A., DE SANTIS C., et al.
2006A&A...454..423V viz 15       D               926 193 The great observatories origins deep survey . VLT/FORS2 spectroscopy in the GOODS-South Field: Part II. VANZELLA E., CRISTIANI S., DICKINSON M., et al.
2007AJ....134..169X viz 15       D               1 116 20 Redshifts of emission-line objects in the Hubble Ultra Deep Field. XU C., PIRZKAL N., MALHOTRA S., et al.
2008A&A...478...83V viz 15       D               885 308 The Great Observatories Origins Deep Survey. VLT/FORS2 spectroscopy in the GOODS-South field: Part III. VANZELLA E., CRISTIANI S., DICKINSON M., 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.
2009A&A...495...53L viz 15       D               1 19223 81 Physical properties of galaxies and their evolution in the VIMOS VLT deep survey. I. The evolution of the mass-metallicity relation up to z ∼ 0.9. LAMAREILLE F., BRINCHMANN J., CONTINI T., et al.
2009AJ....138.1022S viz 15       D               1 198 23 Emission-line galaxies from the Hubble space telescope probing evolution and reionization spectroscopically (PEARS) grism survey. I. The South fields. STRAUGHN A.N., PIRZKAL N., MEURER G.R., et al.
2011AJ....141...64X viz 15       D               1 78 15 Spectroscopic study of the HST/ACS PEARS emission-line galaxies. XIA L., MALHOTRA S., RHOADS J., et al.
2012MNRAS.425.2116C viz 15       D               4 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.
2013ApJ...772...48P viz 16       D               1 888 41 Emission-line galaxies from the Hubble space telescope probing evolution and reionization spectroscopically (PEARS) grism survey. II. The complete sample. PIRZKAL N., ROTHBERG B., LY C., et al.
2013A&A...559A..14L viz 16       D               1 37850 306 The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z ∼ 6.7 selected with 17.5 ≤ iAB≤ 24.75. LE FEVRE O., CASSATA P., CUCCIATI O., et al.
2014ApJS..214...24S viz 16       D               1 66903 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.
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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