Exploratory Chandra observations of the three highest redshift quasars known

被引:67
作者
Brandt, WN [1 ]
Schneider, DP
Fan, XH
Strauss, MA
Gunn, JE
Richards, GT
Anderson, SF
Vanden Berk, DE
Bahcall, NA
Brinkmann, J
Brunner, R
Chen, B
Hennessy, GS
Lamb, DQ
Voges, W
York, DG
机构
[1] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA
[2] Princeton Univ Observ, Princeton, NJ 08540 USA
[3] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[4] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[5] Apache Point Observ, Sunspot, NM 88349 USA
[6] CALTECH, Dept Astron, Pasadena, CA 91125 USA
[7] European Space Agcy VILSPA, XMM Sci Operat Ctr, E-28080 Madrid, Spain
[8] USN Observ, Washington, DC 20392 USA
[9] Univ Chicago, Ctr Astron & Astrophys, Chicago, IL 60637 USA
[10] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
关键词
galaxies : active; galaxies : nuclei; quasars : general; quasars : individual (SDSS J083643.85+005453.3; SDSS J130608.26+035626.3; SDSS J130608.26+035626.3); X-rays : galaxies;
D O I
10.1086/340581
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on exploratory Chandra observations of the three highest redshift quasars known (z = 5.82, 5.99, and 6.28), all found in the Sloan Digital Sky Survey. These data, combined with a previous XMM-Newton observation of a z = 5.74 quasar, form a complete set of color-selected, z > 5.7 quasars. X- ray emission is detected from all of the quasars at levels that indicate that the X-ray-to-optical flux ratios of z approximate to 6, optically selected quasars are similar to those of lower redshift quasars. The observations demonstrate that it will be feasible to obtain quality X-ray spectra of z approximate to 6 quasars with current and future X- ray missions.
引用
收藏
页码:L5 / L9
页数:5
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