|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| [MBR2003] CDFS-H 3771 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST03:59:54 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2003A&A...403..493M |
4820 | 24 | H-band observations of the Chandra Deep Field South. | MOY E., BARMBY P., RIGOPOULOU D., et al. | |||||
|
2007A&A...465.1099R |
693 | 107 | New spectroscopic redshifts from the CDFS and a test of the cosmological relevance of the GOODS-South field. | RAVIKUMAR C.D., PUECH M., FLORES H., et al. | |||||
|
2012MNRAS.425.2116C |
15 | D | 2 | 7382 | 55 | The Arizona CDFS Environment Survey (ACES): A Magellan/IMACS spectroscopic survey of the Chandra Deep Field-South. | COOPER M.C., YAN R., DICKINSON M., 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..224...15X |
16 | D | 1 | 1499 | 121 | The 2 Ms Chandra Deep Field-North survey and the 250 Ks Extended Chandra Deep Field-South survey: improved point-source catalogs. | XUE Y.Q., LUO B., BRANDT W.N., et al. | ||
|
2018MNRAS.475.5133R |
16 | D | 1 | 11242 | 2 | Testing the hierarchical assembly of massive galaxies using accurate merger rates out to z ∼ 1.5. | RODRIGUES M., PUECH M., FLORES H., 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. | ||
|
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. |