Discovery of a z=6.17 galaxy from CFHT and VLT observations

被引:49
作者
Cuby, JG
Le Fèvre, O
McCracken, H
Cuillandre, JC
Magnier, E
Meneux, B
机构
[1] European So Observ, Santiago 19, Chile
[2] Lab Astrophys Marseille, Marseille, France
[3] Osservatorio Astron Bologna, Bologna, Italy
[4] Canada France Hawaii Telescope Corp, Kamuela, HI 96743 USA
关键词
galaxies : high-redshift; early Universe; techniques : spectroscopic;
D O I
10.1051/0004-6361:20030760
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a galaxy at a redshift z = 6.17 identified from deep narrow band imaging and spectroscopic follow-up in one of the CFHT-VIRMOS deep survey fields at 0226-04. In addition to the existing deep BVRI images of this field, we obtained a very deep narrow band image at 920 nm with the aim of detecting Lyalpha emission at redshift similar to6.5. Spectroscopic follow-up of some of the candidates selected on the basis of their excess flux in the NB920 filter was performed at the VLT-UT4 with the FORS2 instrument. For one object a strong and asymmetric emission line associated with a strong break in continuum emission is identified as Lyalpha at z = 6.17. This galaxy was selected from its continuum emission in the 920 nm filter and not from its Lyalpha emission, in effect performing a Lyman Break detection at z = 6.17. We estimate a star formation rate of several tens of M. yr(-1) for this object, with a velocity dispersion similar to400 km s(-1). The spectroscopic follow-up of other high z galaxy candidates is on-going.
引用
收藏
页码:L19 / L22
页数:4
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