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| ZFOURGE CDFS 25490 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.17CEST01:41:15 |
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More on score
| 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. | ||
|
2005ApJ...635..243F
|
15 | D | 251 | 62 | Evolution of field early-type galaxies: the view from GOODS CDFS. | FERRERAS I., LISKER T., CAROLLO C.M., et al. | |||
|
2009ApJ...706..158F
|
15 | D | 1 | 235 | 24 | Early-type galaxies in the PEARS survey: probing the stellar populations at moderate redshift. | FERRERAS I., PASQUALI A., MALHOTRA 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. | ||
|
2013MNRAS.435.1186S
|
16 | D | 1 | 1110 | 8 | Magnitude and size evolution of bulgeless galaxies. | SACHDEVA S. | ||
|
2015AJ....149..178M
|
16 | D | 1 | 1020 | 31 | A WFC3 grism emission line redshift catalog in the GOODS-South field. | MORRIS A.M., KOCEVSKI D.D., TRUMP J.R., 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 | 67524 | 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. |
