Anon J033232-2753 , the SIMBAD biblio

Anon J033232-2753 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST03:10:51


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Title First 3 Authors
2002IAUC.7981....1G 13 6 Supernovae 2002ez, 2002fv, 2002fw, 2002fx, 2002fy, 2002fz, 2002ga. GIAVALISCO M., RIESS A., CASERTANO S., 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.
2005ApJ...635.1022C 109 14 Dust in the host galaxies of supernovae. CHARY R., DICKINSON M.E., TEPLITZ H.I., 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...469..483R 43 12 Unravelling the morphologies of luminous compact galaxies using the HST/ACS GOODS survey. RAWAT A., KEMBHAVI A.K., HAMMER F., 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.
2009PASJ...61..177B viz 15       D               1 258 10 Deep 15 mu.m AKARI observations in the CDFS: Estimating dust luminosities for a MIR-selected sample and for Lyman Break Galaxies and the evolution of Ldust/LUV with the redshift. BURGARELLA D., BUAT V., TAKEUCHI T.T., et al.
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.
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.
2012MNRAS.426..360V 15       D               2 87 15 The spectral energy distributions, host galaxies and environments of variability-selected active galactic nuclei in GOODS-South. VILLFORTH C., SARAJEDINI V. and KOEKEMOER A.
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.
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.
2017MNRAS.467.1965H viz 16       D               1 590 79 The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z ~= 0.9 galaxies. HARRISON C.M., JOHNSON H.L., SWINBANK A.M., et al.
2018A&A...611A..53J viz 16       D               1 24519 3 Automated reliability assessment for spectroscopic redshift measurements. JAMAL S., LE BRUN V., LE FEVRE O., 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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