CANDELS UDS F160W J021735.33-051032.4 , the SIMBAD biblio

CANDELS UDS F160W J021735.33-051032.4 , the SIMBAD biblio (14 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:58:41


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Title First 3 Authors
2012MNRAS.422.1425C 96       D       C       1 11 109 A remarkably high fraction of strong Lyα emitters amongst luminous redshift 6.0 < z < 6.5 Lyman-break galaxies in the UKIDSS Ultra-Deep Survey. CURTIS-LAKE E., McLURE R.J., PEARCE H.J., et al.
2013MNRAS.429..302C 976       D     X   F     25 16 44 The ages, masses and star formation rates of spectroscopically confirmed z ∼ 6 galaxies in CANDELS. CURTIS-LAKE E., McLURE R.J., DUNLOP J.S., et al.
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.
2013ApJ...772...99J 15       D               1 68 51 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. I. Basic characteristics of the rest-frame UV continuum and Lyα emission. JIANG L., EGAMI E., MECHTLEY M., et al.
2013ApJ...773..153J 77               F     1 46 42 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. II. Morphology of the rest-frame UV continuum and Lyα emission. JIANG L., EGAMI E., FAN X., 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...816...16J 16       D               3 44 23 Physical properties of spectroscopically confirmed galaxies at z ≥ 6. III. Stellar populations from SED modeling with secure Lyα emission and redshifts. JIANG L., FINLATOR K., COHEN S.H., 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.
2018A&A...619A.147P 16       D               1 73 67 CANDELSz7: a large spectroscopic survey of CANDELS galaxies in the reionization epoch. PENTERICCI L., VANZELLA E., CASTELLANO M., et al.
2018PASJ...70S..10O viz 16       D               1 365 182 Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4-7 derived with the half-million dropouts on the 100 deg2 sky. ONO Y., OUCHI M., HARIKANE Y., et al.
2020ApJ...889...90J 305       D     X C       7 8 ~ Luminous Lyα emitters with very blue UV-continuum slopes at redshift 5.7 <= z <= 6.6. JIANG L., COHEN S.H., WINDHORST R.A., et al.
2021MNRAS.504.3662L viz 17       D               1 63 10 The size and pervasiveness of Ly α-UV spatial offsets in star-forming galaxies at z ∼ 6. LEMAUX B.C., FULLER S., BRADAC M., 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.
2024ApJ...971..161M 18       D               2 39 ~ SERENADE. II. An ALMA Multiband Dust Continuum Analysis of 28 Galaxies at 5 < z < 8 and the Physical Origin of the Dust Temperature Evolution. MITSUHASHI I., HARIKANE Y., BAUER F.E., et al.

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