Submillimeter properties of the 1 Ms Chandra Deep Field-North X-ray sample

被引:36
作者
Barger, AJ
Cowie, LL
Steffen, AT
Hornschemeier, AE
Brandt, WN
Garmire, GP
机构
[1] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[2] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA
[3] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA
关键词
cosmology : observations; galaxies : active; galaxies : evolution; galaxies : formation;
D O I
10.1086/324062
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present submillimeter observations for 135 of the 370 X-ray sources detected in the 1 Ms exposure of the Chandra Deep Field-North. Nine of the X-ray sources are significantly detected in the submillimeter. The error-weighted mean 850 mum flux is significant at 1.21 +/-0.27 mJy. This value shows little dependence on the 2-8 keV flux from 5x10(-16) to 10(-14) ergs cm(-2) s(-1), but sources with brighter X-ray fluxes than this appear weak in the submillimeter. The ensemble of X-ray sources contribute about 15% of the extragalactic background light at 850 mum. The submillimeter excess is found to be strongest in the optically faint X-ray sources that are also seen at 20 cm, which is consistent with these X-ray sources being obscured and at high redshift (z>1).
引用
收藏
页码:L23 / L28
页数:6
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