THE X-RAY PROPERTIES OF TYPICAL HIGH-REDSHIFT RADIO-LOUD QUASARS

THE X-RAY PROPERTIES OF TYPICAL HIGH-REDSHIFT RADIO-LOUD QUASARS

We report spectral, imaging, and variability results from four new XMM-Newton observations and two new Chandra observations of high-redshift (z ≳4) radio-loud quasars (RLQs). Our targets span lower, and more representative, values of radio loudness than those of past samples of high-redshift RLQs st...

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Bibliographic Details
Main Authors:	Saez, C. (Author), Brandt, W. N. (Author), Shemmer, O. (Author), Chomiuk, L. (Author), Lopez, Laura A. (Author), Miller, B. P. (Author), Vignali, C. (Author), Marshall, Herman (Author)
Other Authors:	MIT Kavli Institute for Astrophysics and Space Research (Contributor), Marshall, Herman Lee (Contributor)
Format:	Article
Language:	English
Published:	IOP Publishing, 2015-02-26T15:26:25Z.
Subjects:	Article
Online Access:	Get fulltext

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