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| EGSIRAC J141716.20+522421.4 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST23:41:18 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2002ApJ...571..136I 
|
158 | 151 | The DEEP Groth Strip survey. X. Number density and luminosity function of field E/S0 galaxies at z < 1. | IM M., SIMARD L., FABER S.M., et al. | |||||
|
2002ApJS..142....1S
|
15 | D | 1 | 7449 | 389 | The DEEP Groth Strip Survey. II. Hubble Space Telescope structural parameters of galaxies in the Groth Strip. | SIMARD L., WILLMER C.N.A., VOGT N.P., et al. | ||
| 2003ApJ...597..239G | 41 | 112 | The DEEP Groth Strip Survey. IX. Evolution of the fundamental plane of field galaxies. | GEBHARDT K., FABER S.M., KOO D.C., et al. | |||||
| 2005ApJ...620..595W | 863 | 158 | The DEEP Groth Strip galaxy redshift survey. III. Redshift catalog and properties of galaxies. | WEINER B.J., PHILLIPS A.C., FABER S.M., et al. | |||||
|
2005ApJS..157..175K
|
95 | 35 | The DEEP Groth Strip Survey. VIII. The evolution of luminous field bulges at redshift z ∼ 1. | KOO D.C., SIMARD L., WILLMER C.N.A., et al. | |||||
|
2007MNRAS.382..109T
|
15 | D | 800 | 448 | Strong size evolution of the most massive galaxies since z ∼ 2. | TRUJILLO I., CONSELICE C.J., BUNDY K., et al. | |||
|
2011ApJS..193...30B
|
15 | D | 1 | 7611 | 103 | UV-to-FIR analysis of Spitzer/IRAC sources in the Extended Groth Strip. II. Photometric redshifts, stellar masses, and star formation rates. | BARRO G., PEREZ-GONZALEZ P.G., GALLEGO J., et al. | ||
|
2013ApJS..204...21M
|
16 | D | 1 | 34882 | 13 | Extended photometry for the DEEP2 galaxy redshift survey: a testbed for photometric redshift experiments. | MATTHEWS D.J., NEWMAN J.A., COIL A.L., et al. | ||
| 2015MNRAS.454.1332S | 16 | D | 1 | 155 | 11 | Observed trend in the star formation history and the dark matter fraction of galaxies at redshift z ∼ 0.8. | SHETTY S. and CAPPELLARI M. |
