VUDS 534052568 , the SIMBAD biblio

VUDS 534052568 , the SIMBAD biblio (29 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST04:41:47


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Title First 3 Authors
2004MNRAS.353...30C 31 28 A deeper view of extremely red galaxies: the redshift distribution in the GOODS/CDFS ISAAC field. CAPUTI K.I., DUNLOP J.S., McLURE R.J., 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.
2015ApJ...803...34B viz 16       D               1 10313 1045 UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields. BOUWENS R.J., ILLINGWORTH G.D., OESCH P.A., 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.
2017A&A...600A.110T viz 16       D               1 700 92 The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to zspec ∼ 6 in CANDELS. TASCA L.A.M., LE FEVRE O., RIBEIRO B., 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 25243 42 HDUV: the Hubble Deep UV Legacy Survey. OESCH P.A., MONTES M., REDDY N., et al.
2020ApJ...891...69C 16       D               2 22 ~ On the absence of high-redshift AGNs: little growth in the supermassive black hole population at high redshifts. COWIE L.L., BARGER A.J., BAUER F.E., et al.
2020MNRAS.496..695C viz 263       D S   X C       5 154 49 Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5. CARNALL A.C., WALKER S., McLURE R.J., et al.
2021ApJS..257...68S viz 17       D               1 9083 17 The Spitzer/IRAC Legacy over the GOODS fields: full-depth 3.6, 4.5, 5.8, and 8.0 µm mosaics and photometry for >9000 galaxies at z ∼ 3.5-10 from the GOODS Reionization Era wide-Area Treasury from Spitzer (GREATS). STEFANON M., LABBE I., OESCH P.A., et al.
2023MNRAS.520.3974C 89           X         2 17 35 A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS. CARNALL A.C., McLEOD D.J., McLURE R.J., et al.
2023Natur.619..716C 2333     A     X C       53 2 ~ A massive quiescent galaxy at redshift 4.658. CARNALL A.C., McLURE R.J., DUNLOP J.S., et al.
2023A&A...678L...9D 548     A     X C       12 5 ~ The [CII] 158 μm emission line as a gas mass tracer in high redshift quiescent galaxies. D'EUGENIO C., DADDI E., LIU D., et al.
2024MNRAS.527.7965W 269           X         6 3 ~ First Light and Reionization Epoch Simulations (FLARES) - XIV. The Balmer/4000 Å breaks of distant galaxies. WILKINS S.M., LOVELL C.C., IRODOTOU D., et al.
2024A&A...683L...4J 45           X         1 14 ~ Cosmic Vine: A z = 3.44 large-scale structure hosting massive quiescent galaxies. JIN S., SILLASSEN N.B., MAGDIS G.E., et al.
2024MNRAS.531.3187M 45           X         1 30 ~ The origin of large emission line widths in massive galaxies at redshifts z ∼ 3-4. MARTINEZ-MARIN M., GLAZEBROOK K., NANAYAKKARA T., et al.
2024ApJ...969L..13W 90             C       1 7 ~ RUBIES: Evolved Stellar Populations with Extended Formation Histories at z ∼ 7-8 in Candidate Massive Galaxies Identified with JWST/NIRSpec. WANG B., LEJA J., DE GRAAFF A., et al.
2024ApJ...971...47F 90           X         2 2 ~ Dead or Alive? How Bursty Star Formation and Patchy Dust Can Cause Temporary Quiescence in High-redshift Galaxies. FAISST A.L. and MORISHITA T.
2024MNRAS.534..325C 1003       D     X C F     21 8 ~ The JWST EXCELS survey: too much, too young, too fast? Ultra-massive quiescent galaxies at 3 < z < 5. CARNALL A.C., CULLEN F., McLURE R.J., et al.
2024ApJ...976...33L 45           X         1 3 ~ Fast Outflow in the Host Galaxy of the Luminous z = 7.5 Quasar J1007+2115. LIU W., FAN X., YANG J., et al.
2025MNRAS.536.3554X 93             C       1 187 ~ Cosmic quenching and scaling laws for the evolution of supermassive black holes and host galaxies. XU Z.
2025ApJ...978...90A 93           X         2 4 ~ The FENIKS Survey: Spectroscopic Confirmation of Massive Quiescent Galaxies at z ∼ 3-5. ANTWI-DANSO J., PAPOVICH C., ESDAILE J., et al.
2025MNRAS.538.1501I 187           X         4 3 ~ Black hole mass of a quiescent galaxy hosting a Type 1 AGN at z = 2.09: implications for black hole-galaxy coevolution and AGN quenching at high redshift. ITO K., TANAKA T.S., SHIMASAKU K., et al.
2025A&A...696A..79M 47           X         1 15 ~ A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XVIII. Reconstructing the star formation history of early-type galaxies through the combination of their UV and Hα emission. MARTOCCHIA S., BOSELLI A., MARASTON C., et al.
2025MNRAS.539..557B 93           X         2 23 ~ The abundance and nature of high-redshift quiescent galaxies from JADES spectroscopy and the FLAMINGO simulations. BAKER W.M., LIM S., D'EUGENIO F., et al.
2025NatAs...9.1541O 233           X C       4 4 ~ A post-starburst pathway for the formation of massive galaxies and black holes at z > 6. ONOUE M., DING X., SILVERMAN J.D., et al.
2025MNRAS.544..160D 93               F     1 6 ~ From FFB starbursts at cosmic dawn to quenching at cosmic morning: Hi-z galaxy bimodality. DEKEL A., MANDELKER N., LI Z., et al.
2026ApJ...997...29K 920       D     X C       18 24 ~ Connecting Environment, Star Formation History, and Morphology of Massive Quiescent Galaxies at 3 < z < 4 with JWST. KAWINWANICHAKIJ L., GLAZEBROOK K., NANAYAKKARA T., et al.
2026ApJ...998..239J 1280     A S   X C       24 4 ~ JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z = 5 to z = 0.5. JI Z., WILLIAMS C.C., SUESS K.A., et al.

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