GOODS-MUSIC 8339 , the SIMBAD biblio

GOODS-MUSIC 8339 , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST14:20:31

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
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.
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.
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.
2009AJ....138.1022S viz 15       D               1 198 23 Emission-line galaxies from the Hubble space telescope probing evolution and reionization spectroscopically (PEARS) grism survey. I. The South fields. STRAUGHN A.N., PIRZKAL N., MEURER G.R., et al.
2013ApJ...772...48P viz 16       D               1 888 41 Emission-line galaxies from the Hubble space telescope probing evolution and reionization spectroscopically (PEARS) grism survey. II. The complete sample. PIRZKAL N., ROTHBERG B., LY C., et al.
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.
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 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.
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.
2019A&A...624A.141U viz 17       D               2 1907 76 The MUSE-Wide Survey: survey description and first data release. URRUTIA T., WISOTZKI L., KERUTT J., et al.
2021MNRAS.503.1753S viz 17       D               1 345 10 Flat rotation curves of z ∼ 1 star-forming galaxies. SHARMA G., SALUCCI P., HARRISON C.M., et al.
2022A&A...659A..40S viz 18       D               1 225 9 Observational evidence of evolving dark matter profiles at z ≤ 1. SHARMA G., SALUCCI P. and VAN DE VEN G.

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