Very high redshift X-ray-selected active galactic nuclei in the Chandra Deep Field-North

被引:59
|
作者
Barger, AJ
Cowie, LL
Capak, P
Alexander, DM
Bauer, FE
Brandt, WN
Garmire, GP
Hornschemeier, AE
机构
[1] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA
[2] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 USA
[3] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[4] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA
[5] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
来源
ASTROPHYSICAL JOURNAL | 2003年 / 584卷 / 02期
关键词
cosmology : observations; galaxies : active; galaxies : distances and redshifts; galaxies : evolution; galaxies : formation;
D O I
10.1086/368407
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Deep Chandra X-ray exposures provide an efficient route for locating optically faint active galactic nuclei (AGNs) at high redshifts. We use deep multicolor optical data to search for z > 5 AGNs in the 2 Ms X-ray exposure of the Chandra Deep Field-North. Of the 423 X-ray sources bright enough (z' < 25.2) for a color-color analysis, at most one lies at z = 5-6, and none at z > 6. The one z > 5 object is spectroscopically confirmed at z = 5.19. Only 31 of the 77 sources with z' > 25.2 are undetected in the B or V bands at the 2 sigma level and could lie at z > 5. There are too few moderate-luminosity AGNs at z = 5-6.5 to ionize the intergalactic medium.
引用
收藏
页码:L61 / L64
页数:4
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