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[TCB2007] 12004496 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST04:53:31 |
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. | ||
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. | |||
2011ApJ...728...38Y | 15 | D | 1 | 377 | 67 | AEGIS: demographics of X-ray and optically selected active galactic nuclei. | YAN R., HO L.C., NEWMAN J.A., et al. | ||
2012MNRAS.419..687R | 15 | D | 1 | 169 | 71 | Are luminous radio-loud active galactic nuclei triggered by galaxy interactions? | RAMOS ALMEIDA C., BESSIERE P.S., TADHUNTER C.N., et al. | ||
2012ApJ...751...50G | 15 | D | 1 | 8632 | 29 | The DEEP2 Galaxy Redshift Survey: the Voronoi-Delaunay method catalog of galaxy groups. | GERKE B.F., NEWMAN J.A., DAVIS M., 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. | ||
2013MNRAS.436..997R | 16 | D | 1 | 191 | 28 | The environments of luminous radio galaxies and type-2 quasars. | RAMOS ALMEIDA C., BESSIERE P.S., TADHUNTER C.N., et al. | ||
2019A&A...631A...9B | 17 | D | 1 | 8367 | ~ | The OTELO survey. I. Description, data reduction, and multi-wavelength catalogue. | BONGIOVANNI A., RAMON-PEREZ M., PEREZ GARCIA A.M., et al. | ||
2021A&A...647A..89N | 17 | D | 1 | 3659 | ~ | The OTELO survey as a morphological probe. Last ten Gyr of galaxy evolution. The mass-size relation up to z = 2. | NADOLNY J., BONGIOVANNI A., CEPA J., et al. |