CANDELS UDS F160W J021735.91-050810.8 , the SIMBAD biblio

CANDELS UDS F160W J021735.91-050810.8 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST10:04:38


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Title First 3 Authors
2013ApJS..206...10G viz 15       D               1 34915 252 CANDELS multiwavelength catalogs: source identification and photometry in the CANDELS UKIDSS ultra-deep survey field. GALAMETZ A., GRAZIAN A., FONTANA A., et al.
2014ApJ...783L..14S 18       D               1 21 167 A substantial population of massive quiescent galaxies at z ∼ 4 from ZFOURGE. STRAATMAN C.M.S., LABBE I., SPITLER L.R., 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...808L..29S 16       D               1 31 42 The sizes of massive quiescent and star-forming galaxies at z ∼ 4 with ZFOURGE and CANDELS. STRAATMAN C.M.S., LABBE I., SPITLER L.R., 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.
2019MNRAS.483.3060G viz 16       D               3 269 6 Candidate massive galaxies at z ∼ 4 in the Dark Energy Survey. GUARNIERI P., MARASTON C., THOMAS D., et al.
2020MNRAS.496..695C viz 16       D               1 154 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.
2024MNRAS.534..325C 1048       D     X C       23 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.
2025ApJ...988L..19J 159       D     X         4 6 ~ Explaining Ultramassive Quiescent Galaxies at 3 < z < 5 in the Context of Their Environments. JESPERSEN C.K., CARNALL A.C. and LOVELL C.C.
2025A&A...701A.168D 47           X         1 7 ~ A remarkable ruby: Absorption in dense gas, rather than evolved stars, drives the extreme Balmer break of a little red dot at z = 3.5. DE GRAAFF A., RIX H.-W., NAIDU R.P., 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..252Z 20       D               1 20 ~ RUBIES Spectroscopically Confirms the High Number Density of Quiescent Galaxies from 2 < z< 5. ZHANG Y., DE GRAAFF A., SETTON D.J., et al.

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