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VCDFS 38853 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.03.28CET20:13:41 |
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 |
---|---|---|---|---|---|---|---|---|---|
2002A&A...392..741G | 1405 | 34 | ESO Imaging Survey. The stellar catalogue in the Chandra Deep Field South. | GROENEWEGEN M.A.T., GIRARDI L., HATZIMINAOGLOU E., et al. | |||||
2004A&A...428.1043L | 15 | D | 1601 | 300 | The VIMOS VLT Deep Survey. Public release of 1599 redshifts to IAB≤24 across the Chandra Deep Field South. | LE FEVRE O., VETTOLANI G., PALTANI S., et al. | |||
2004ApJ...614..586S | 3 | 17 | 170 | Colors of active galactic nucleus host galaxies at 0.5<z<1.1 from the GEMS survey. | SANCHEZ S.F., JAHNKE K., WISOTZKI L., et al. | ||||
2006AJ....131.2826S | 1 | 110 | 405 | The X-Ray-to-Optical properties of optically selected active galaxies over wide luminosity and redshift ranges. | STEFFEN A.T., STRATEVA I., BRANDT W.N., et al. | ||||
2009A&A...495...53L | 15 | D | 1 | 19223 | 81 | Physical properties of galaxies and their evolution in the VIMOS VLT deep survey. I. The evolution of the mass-metallicity relation up to z ∼ 0.9. | LAMAREILLE F., BRINCHMANN J., CONTINI T., et al. | ||
2012MNRAS.425.2116C | 15 | D | 4 | 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. | ||
2013A&A...559A..14L | 16 | D | 1 | 37850 | 306 | The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z ∼ 6.7 selected with 17.5 ≤ iAB≤ 24.75. | LE FEVRE O., CASSATA P., CUCCIATI O., et al. | ||
2018A&A...611A..53J | 16 | D | 1 | 24519 | 3 | Automated reliability assessment for spectroscopic redshift measurements. | JAMAL S., LE BRUN V., LE FEVRE O., et al. | ||
2018A&A...620A..68H | 58 | D | X | 2 | 101 | 6 | Optical linear polarization measurements of quasars obtained with the Very Large Telescope at Paranal Observatory. | HUTSEMEKERS D., BORGUET B., SLUSE D., et al. |