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The Chandra Deep Field North survey.: VIII.: X-ray constraints on spiral galaxies from 0.4 < z < 1.5

被引：53
作者：
Hornschemeier, AE [1 ]
Brandt, WN
Alexander, DM
Bauer, FE
Garmire, GP
Schneider, DP
Bautz, MW
Chartas, G
机构：
[1] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA
[2] MIT, Ctr Space Res, Cambridge, MA 02139 USA
来源：
ASTROPHYSICAL JOURNAL | 2002年 / 568卷 / 01期
基金：
美国国家科学基金会;
关键词：
cosmology : observations; diffuse radiation; surveys; X-rays : galaxies; X-rays : general;
D O I：
10.1086/338802
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a statistical X-ray study of spiral galaxies in the Hubble Deep Field North and its flanking fields using the Chandra Deep Field North 1 Ms data set. We find that approximate toL* galaxies with 0.4.less than or similar to z less than or similar to 1.5 have X-ray luminosity and ratios of X-ray to B-band luminosity similar to those in the local universe. The data, however, are consistent with an increase in both by a factor of approximate to2-3. We have also determined that typical spiral galaxies at 0.4 less than or similar to z less than or similar to 1.5 should be detected in the 0.5-2 keV band in the flux range (3-6) x 10(-18) erg cm(-2) s(-1).
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页码：82 / 87
页数：6
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