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| GOODS J033239.97-274213.6 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST04:00:34 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2004ApJ...600L..93G 
|
15 | D | 1 | 7819 | 1453 | The Great Observatories Origins Deep Survey: initial results from optical and near-infrared imaging. | GIAVALISCO M., FERGUSON H.C., KOEKEMOER A.M., et al. | ||
| 2009ApJ...695.1315R | 75 | X F | 1 | 25 | 8 | Rest-frame UV versus optical morphologies of galaxies using Sersic profile fitting: the importance of morphological K-correction. | RAWAT A., WADADEKAR Y. and DE MELLO D. | ||
|
2010A&A...512A..12B
|
15 | D | 1 | 4352 | 228 | The Great Observatories Origins Deep Survey. VLT/VIMOS spectroscopy in the GOODS-South field: part II. | BALESTRA I., MAINIERI V., POPESSO P., et al. | ||
|
2011A&A...533A.119E
|
15 | D | 1 | 3965 | 926 | GOODS-Herschel: an infrared main sequence for star-forming galaxies. | ELBAZ D., DICKINSON M., HWANG H.S., et al. | ||
|
2011ApJ...743..146C
|
15 | D | 1 | 4132 | 61 | Active and passive galaxies at z ∼ 2: rest-frame optical morphologies with WFC3. | CAMERON E., CAROLLO C.M., OESCH P.A., 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. | ||
|
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. | ||
|
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. |
