GOODS J033227.11-274643.3 , the SIMBAD biblio

GOODS J033227.11-274643.3 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST11:33:52


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Title First 3 Authors
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.
2013A&A...551A..93G viz 16       D               1 19 24 Magellan/MMIRS near-infrared multi-object spectroscopy of nebular emission from star-forming galaxies at 2 < z < 3. GUAITA L., FRANCKE H., GAWISER E., et al.
2014ApJ...784..152A 16       D               1 58 17 The properties of Hα emission-line galaxies at z = 2.24. AN F.X., ZHENG X.Z., WANG W.-H., 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...817...10G viz 16       D               1 259 10 Young, star-forming galaxies and their local counterparts: the evolving relationship of mass-SFR-metallicity since z ∼ 2.1. GRASSHORN GEBHARDT H.S., ZEIMANN G.R., CIARDULLO R., 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.
2017ApJ...835..116A 16       D               1 58 4 Extinction correction significantly influences the estimate of the Lyα escape fraction. AN F.X., ZHENG X.Z., HAO C.-N., 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.
2018ApJS..237...12O viz 16       D               1 25244 42 HDUV: the Hubble Deep UV Legacy Survey. OESCH P.A., MONTES M., REDDY N., et al.

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