The VIMOS VLT Deep Survey -: Public release of 1599 redshifts to IAB≤24 across the Chandra Deep Field South

被引:280
作者
Le Fèvre, O
Vettolani, G
Paltani, S
Tresse, L
Zamorani, G
Le Brun, V
Moreau, C
Bottini, D
Maccagni, D
Picat, JP
Scaramella, R
Scodeggio, M
Zanichelli, A
Adami, C
Arnouts, S
Bardelli, S
Bolzonella, M
Cappi, A
Charlot, S
Contini, T
Foucaud, S
Franzetti, P
Garilli, B
Gavignaud, I
Guzzo, L
Ilbert, O
Iovino, A
McCracken, HJ
Mancini, D
Marano, B
Marinoni, C
Mathez, G
Mazure, A
Meneux, B
Merighi, R
Pellò, R
Pollo, A
Pozzetti, L
Radovich, M
Zucca, E
Arnaboldi, M
Bondi, M
Bongiorno, A
Busarello, G
Ciliegi, P
Gregorini, L
Mellier, Y
Merluzzi, P
Ripepi, V
Rizzo, D
机构
[1] Univ Aix Marseille 1, OAMP, UMR 6110, Lab Astrophys Marseille, F-13376 Marseille 12, France
[2] IRA, INAF, I-40129 Bologna, Italy
[3] IASF, INAF, I-20133 Milan, Italy
[4] Observ Midi Pyrenees, Astrophys Lab, F-31400 Toulouse, France
[5] Osservatorio Astron Bologna, INAF, I-40127 Bologna, Italy
[6] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
[7] Inst Astrophys Paris, UMR 7095, F-75014 Paris, France
[8] INAF, Osservatorio Astron Brera, I-20121 Milan, Italy
[9] INAF, Osservatorio Astron Capodimonte, I-80131 Naples, Italy
[10] Max Planck Inst Astrophys, D-85741 Garching, Germany
[11] European So Observ, D-85748 Garching, Germany
[12] Observ Paris, LERMA, UMR 8112, F-75014 Paris, France
关键词
surveys; galaxies : high-redshift; galaxies : distances and redshifts; cosmology : observations; galaxies : evolution; cosmology : large scale structure of Universe;
D O I
10.1051/0004-6361:20048072
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper presents the VIMOS VLT Deep Survey around the Chandra Deep Field South (CDFS). We have measured 1599 new redshifts with VIMOS on the European Observatory Very Large Telescope-UT3, in an area 21 x 21.6 arcmin(2), including 784 redshifts in the Hubble Space Telescope-Advanced Camera for Surveys GOODS area. 30% of all objects with I-AB = 24 have been observed independently of magnitude, indicating that the sample is purely magnitude limited. We have reached an unprecedented completeness level of 84% in terms of the ratio of secure measurements vs. observed objects, while 95% of all objects have a redshift measurement. A total of 1452 galaxies, 139 stars, 8 QSOs have a redshift identification, 141 of these being unsecure measurements. The redshift distribution down to I-AB = 24 is peaked at a median redshift z = 0.73, with a significant high redshift tail extending up to similar to4. Several high density peaks in the distribution of galaxies are identified. In particular, the strong peak at z = 0.735 contains more than 130 galaxies in a velocity range +/-2000 km s(-1) distributed all across the transverse similar to20 h(-1) Mpc of the survey. We are releasing all redshifts to the community, along with the cross identification with HST-ACS GOODS sources on the CENCOS database environment http://cencosw.oamp.fr.
引用
收藏
页码:1043 / 1049
页数:7
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