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| ZFOURGE CDFS 2345 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST01:45:24 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
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. | |||
|
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 | 1 | 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. | ||
|
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. | ||
|
2017ApJS..228....2L
|
16 | D | 1 | 1061 | 334 | The Chandra Deep Field-South survey: 7 Ms source catalogs. | LUO B., BRANDT W.N., XUE Y.Q., et al. | ||
|
2019ApJ...887...23B
|
17 | D | 1 | 942 | ~ | A submillimeter perspective on the GOODS fields (SUPER GOODS). IV. The submillimeter properties of X-ray sources in the CDF-S. | BARGER A.J., COWIE L.L., BAUER F.E., et al. | ||
|
2020MNRAS.492.1887G
|
17 | D | 1 | 792 | ~ | Physical properties of the CDFS X-ray sources through fitting spectral energy distributions. | GUO X., GU Q., DING N., et al. |
