ZFOURGE CDFS 16818 , the SIMBAD biblio

ZFOURGE CDFS 16818 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST07:07:15


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Title First 3 Authors
2004ApJS..154..501P 43 108 GRAPES, grism spectroscopy of the Hubble Ultra Deep Field: description and data reduction. PIRZKAL N., XU C., MALHOTRA S., et al.
2005AJ....130....1T viz 1285 99 The near-infrared camera and multi-object spectrometer ultra deep field: observations, data reduction, and galaxy photometry. THOMPSON R.I., ILLINGWORTH G., BOUWENS R., et al.
2005ApJ...626..680D 19 13 755 Passively evolving early-type galaxies at 1.4 ≲ z ≲ 2.5 in the Hubble Ultra Deep Field. DADDI E., RENZINI A., PIRZKAL N., et al.
2006A&A...452..119O viz 3542 8 ESO imaging survey: infrared observations of CDF-S and HDF-S. OLSEN L.F., MIRALLES J.-M., DA COSTA L., et al.
2006AJ....132..926C viz 15       D               2664 396 Galaxies in the Hubble Ultra Deep Field. I. Detection, multiband photometry, photometric redshifts, and morphology. COE D., BENITEZ N., SANCHEZ S.F., et al.
2006ApJ...639..731C 47 18 Clues to active galactic nucleus growth from optically variable objects in the Hubble Ultra Deep Field. COHEN S.H., RYAN R.E.Jr, STRAUGHN A.N., et al.
2006NewAR..50..821W 46 7 Did galaxy assembly and supermassive black-hole growth go hand-in-hand? WINDHORST R.A., COHEN S.H., STRAUGHN A.N., et al.
2007ApJ...668..839R viz 15       D               1309 41 The galaxy luminosity function at z ≃ 1 in the HUDF: probing the dwarf population. RYAN R.E.Jr, HATHI N.P., COHEN S.H., et al.
2008MNRAS.386..909C 114           X   F     2 68 185 The structures of distant galaxies - I. Galaxy structures and the merger rate to z ∼ 3 in the Hubble Ultra-Deep Field. CONSELICE C.J., RAJGOR S. and MYERS R.
2011ApJ...735L..22S viz 15       D               1 130 60 Morphological evolution of galaxies from ultra-deep Hubble Space Telescope Wide Field Camera 3 imaging: the Hubble sequence at z ∼ 2. SZOMORU D., FRANX M., BOUWENS R.J., et al.
2009RAA.....9...59F 318       D     X C F     7 27 14 Classification of extremely red objects in the Hubble Ultra Deep Field. FANG G.-W., KONG X. and WANG M.
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.
2013A&A...549A..63K viz 16       D               1 245 70 GMASS ultradeep spectroscopy of galaxies at z ∼ 2. VII. Sample selection and spectroscopy. KURK J., CIMATTI A., DADDI E., 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.
2015ApJ...805..181C viz 16       D               1 135 23 A physical approach to the identification of high-z mergers: morphological classification in the stellar mass domain. CIBINEL A., FLOC'H E.L., PERRET V., et al.
2015AJ....150...31R viz 16       D               1 9969 140 UVUDF: ultraviolet through near-infrared catalog and photometric redshifts of galaxies in the Hubble Ultra Deep Field. RAFELSKI M., TEPLITZ H.I., GARDNER J.P., 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 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.
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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