EIS-DEEP CDFS-2 J 1 187 , the SIMBAD biblio

EIS-DEEP CDFS-2 J 1 187 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST14:50:17


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Title First 3 Authors
2002A&A...392..395C viz 546 166 The K20 survey. III. Photometric and spectroscopic properties of the sample. CIMATTI A., MIGNOLI M., DADDI E., et al.
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...437..883M viz 15       D               1 546 208 The K20 survey. VII. The spectroscopic catalogue: Spectral properties and evolution of the galaxy population. MIGNOLI M., CIMATTI A., ZAMORANI G., et al.
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...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.
2007A&A...472..455N 116 25 Presence of dust with a UV bump in massive, star-forming galaxies at 1 < z < 2.5. NOLL S., PIERINI D., PANNELLA M., et al.
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.
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               10 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.
2012A&A...545A.141B viz 15       D               1 751 150 GOODS-Herschel: dust attenuation properties of UV selected high redshift galaxies. BUAT V., NOLL S., BURGARELLA D., et al.
2013A&A...559A..14L viz 15       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 15       D               1 97940 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.
2015AJ....149..178M viz 16       D               1 1020 31 A WFC3 grism emission line redshift catalog in the GOODS-South field. MORRIS A.M., KOCEVSKI D.D., TRUMP J.R., 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.
2021ApJ...923..203S viz 17       D               1 235 30 CLEAR: the gas-phase metallicity gradients of star-forming galaxies at 0.6 < z < 2.6. SIMONS R.C., PAPOVICH C., MOMCHEVA I., et al.
2023ApJ...943...37B viz 17       D               1 221 3 CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at 0.6 < z < 1.3. BACKHAUS B.E., BRIDGE J.S., TRUMP J.R., et al.

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