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| CANDELS UDS F160W J021702.13-051356.2 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:25:05 |
| 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 |
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 |
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 |
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...618A..85S |
21 | D | 2 | 24 | 140 | Near infrared spectroscopy and star-formation histories of 3 ≤ z ≤ 4 quiescent galaxies. | SCHREIBER C., GLAZEBROOK K., NANAYAKKARA T., et al. | ||
| 2025MNRAS.537.1826T | 93 | X | 2 | 11 | ~ | Age-dating early quiescent galaxies: high star formation efficiency, but consistent with direct, higher-redshift observations. | TURNER C., TACCHELLA S., D'EUGENIO F., et al. | ||
| 2025ApJ...981...78N | 159 | D | X | 4 | 22 | ~ | The Formation Histories of Massive and Quiescent Galaxies in the 3 < z < 4.5 Universe. | NANAYAKKARA T., GLAZEBROOK K., SCHREIBER C., et al. | |
| 2026ApJ...997...29K | 720 | D | X | 15 | 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...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. |