CANDELS UDS F160W J021738.59-050746.9 , the SIMBAD biblio

CANDELS UDS F160W J021738.59-050746.9 , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST04:12:11

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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
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.
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.
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.
2017Msngr.167...31M viz 16       D               1 879 3 VANDELS: Exploring the physics of high-redshift galaxy evolution. McLURE R., PENTERICCI L. (The VANDELS Team)
2021A&A...647A.150G viz 17       D               1 2166 44 The VANDELS ESO public spectroscopic survey. Final data release of 2087 spectra and spectroscopic measurements. GARILLI B., McLURE R., PENTERICCI L., et al.
2022ApJS..259...20H viz 17       D               1 1042 83 GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. HARIKANE Y., ONO Y., OUCHI M., et al.
2023A&A...678A..25T viz 17       D               1 1733 ~ The VANDELS ESO public spectroscopic survey: The spectroscopic measurements catalogue. TALIA M., SCHREIBER C., GARILLI B., et al.
2025ApJ...986..165T 19       D               1 66 ~ Broad-line AGNs at 3.5 < z < 6: The Black Hole Mass Function and a Connection with Little Red Dots. TAYLOR A.J., FINKELSTEIN S.L., KOCEVSKI D.D., et al.
2025A&A...701A.168D 4273     A     X C       91 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.
2025A&A...702A..57H viz 47           X         1 8 ~ RUBIES: A spectroscopic census of little red dots All point sources with v-shaped continua have broad lines. HVIDING R.E., DE GRAAFF A., MILLER T.B., et al.
2025ApJ...994..113L 280           X C       5 6 ~ The Balmer Break and Optical Continuum of Little Red Dots from Super-Eddington Accretion. LIU H., JIANG Y.-F., QUATAERT E., et al.
2026ApJ...998L...4S 300           X C       5 4 ~ Evolutionary Tracks and Spectral Properties of Quasi-stars and Their Correlation with Little Red Dots. SANTARELLI A.D., FARAG E., BELLINGER E.P., et al.
2026ApJ...998..124N 450           X C       8 1 ~ Supermassive Stars Match the Spectral Signatures of JWST's Little Red Dots. NANDAL D. and LOEB A.
2026ApJ...998..148J 50           X         1 3 ~ Little Red Dots and Their Progenitors from Direct Collapse Black Holes. JEON J., LIU B., BROMM V., et al.
2026ApJ..1000...90I 250           X C       4 5 ~ Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts. INAYOSHI K., MURASE K. and KASHIYAMA K.

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