ZFOURGE CDFS 27838 , the SIMBAD biblio

ZFOURGE CDFS 27838 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:08:12


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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.
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.
2009ApJ...695.1315R 187           X C F     3 25 8 Rest-frame UV versus optical morphologies of galaxies using Sersic profile fitting: the importance of morphological K-correction. RAWAT A., WADADEKAR Y. and DE MELLO D.
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.
2015A&A...580A..42K 16       D               1 54 9 Emission-line-selected galaxies at z = 0.6-2 in GOODS South: Stellar masses, SFRs, and large-scale structure. KOCHIASHVILI I., MOLLER P., MILVANG-JENSEN B., et al.
2016A&A...591A.151G 16       D               1 48 3 Properties of galaxies at the faint end of the Hα luminosity function at z ∼ 0.62. GOMEZ-GUIJARRO C., GALLEGO J., VILLAR V., 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.
2018MNRAS.478.4416R viz 16       D               1 139 1 Classifying galaxy spectra at 0.5 < z < 1 with self-organizing maps. RAHMANI S., TEIMOORINIA H. and BARMBY P.

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