A wide-field spectroscopic survey of the cluster of galaxies C10024+1654 - I. The catalogue

被引:65
作者
Czoske, O
Kneib, JP
Soucail, G
Bridges, TJ
Mellier, Y
Cuillandre, JC
机构
[1] Observ Midi Pyrenees, UMR5572, F-31400 Toulouse, France
[2] Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England
[3] Inst Astrophys, F-75014 Paris, France
[4] Canada France Hawaii Telescope Corp, Kamuela, HI 96743 USA
[5] Observ Paris, DEMIRM, F-75014 Paris, France
关键词
galaxies : clusters : Cl0024+1654; cosmology : observations; cosmology : large-scale structure of the Universe;
D O I
10.1051/0004-6361:20010398
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the catalogue of a wide-field CFHT/WHT spectroscopic survey of the lensing cluster Cl0024+1654 at z = 0.395. This catalogue contains 618 new spectra, of which 581 have identified redshifts. Adding redshifts available from the literature, the final catalogue contains data for 687 objects with redshifts identified for 650 of them. 295 galaxies have redshifts in the range 0.37 < z < 0.41, i.e. are cluster members or lie in the immediate neighbourhood of the cluster. The area covered by the survey is 21 x 25 arcmin(2) in size, corresponding to 4 x 4.8 h(-2) Mpc(2) at the cluster redshift. The survey is 45% complete down to V = 22 over the whole field covered; within 3 arcmin of the cluster centre the completeness exceeds 80% at the same magnitude. A detailed completeness analysis is presented. The catalogue gives astrometric position, redshift, V magnitude and V-I colour, as well as the equivalent widths for a number of lines. Apart from the cluster Cl0024+1654 itself, three other structures are identified in redshift space. a group of galaxies at z = 0.38, just in front of Cl0024+1654 and probably interacting with it, a close pair of groups of galaxies at z similar to 0.495 and an overdensity of galaxies at z similar to 0.18 with no obvious centre. The spectroscopic catalogue will be used to trace the three-dimensional structure of the cluster Cl0024+1654 as well as study the physical properties of the galaxies in the cluster and in its environment.
引用
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页码:391 / 405
页数:15
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