[ITAL]Chandra[/ITAL] Detection of Highest Redshift ([CLC][ITAL]z[/ITAL][/CLC] ∼ 6) Quasars in X-Rays
Author(s) -
Smita Mathur,
B. J. Wilkes,
Himel Ghosh
Publication year - 2002
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/340831
Subject(s) - physics , redshift , astrophysics , quasar , rest frame , spectral line , astronomy , galaxy
We report on Chandra observations of three quasars SDSSP J083643+005453,SDSSP J103027+052455, and SDSSP J130608+035626 at redshifts 5.82, 6.28 and 5.99respectively. All the three sources are clearly detected in the X-ray band, upto rest frame energies of ~55 keV. These observations demonstrate theunprecedented sensitivity of Chandra to detect faint sources in relativelyshort exposure times (5.7--8.2 ksec). The broad band X-ray properties of thesehighest redshift quasars do not appear to be any different from their lowerredshift cousins. Spectra of the sources could not be determined with only fewcounts detected. Observations with XMM-Newton will be able to constrain thespectral shapes, if they are simple. Determination of complex spectra in areasonable amount of time, however, will have to await next generation of X-raymissions.Comment: Submitted to ApJ Letter
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