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| CANDELS UDS F160W J021756.32-051407.1 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST02:32:05 |
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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 
|
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. | ||
|
2016ApJS..225...27M
|
16 | D | 1 | 19341 | 548 | The 3D-HST survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for ∼ 100,000 galaxies. | MOMCHEVA I.G., BRAMMER G.B., VAN DOKKUM P.G., et al. | ||
|
2018MNRAS.474.3875B
|
16 | D | 1 | 133173 | 163 | Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3. | BALDRY I.K., LISKE J., BROWN M.J.I., et al. | ||
|
2018A&A...620A...7G
|
16 | D | 1 | 24335 | 10 | The XXL Survey. XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters. | GUGLIELMO V., POGGIANTI B.M., VULCANI B., et al. | ||
|
2020ApJ...905..170M
|
16 | D | 1 | 4760 | 24 | Galaxy sizes since z = 2 from the perspective of stellar mass distribution within galaxies. | MOSLEH M., HOSSEINNEJAD S., HOSSEINI-SHAHISAVANDI S.Z., et al. | ||
|
2022MNRAS.513..439D
|
17 | D | 1 | 302202 | 70 | Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions. | DRIVER S.P., BELLSTEDT S., ROBOTHAM A.S.G., et al. | ||
|
2024A&A...682A.110B
|
18 | D | 1 | 1053 | ~ | Strong size evolution of disc galaxies since z = 1 Readdressing galaxy growth using a physically motivated size indicator. | BUITRAGO F. and TRUJILLO I. |
