X-ray properties of high-redshift Radio Loud and Radio Quiet Quasars observed by Chandra
F. Shaban, A. Siemiginowska, R.M. Suleiman, M. El-Nawawy, A. Ali

TL;DR
This study analyzes high-redshift quasars to compare their X-ray properties, revealing that radio-loud quasars have flatter spectra and higher X-ray luminosity than radio-quiet quasars, using Chandra observations.
Contribution
It provides the first large-scale comparison of X-ray spectral properties between high-redshift RLQ and RQQ, confirming spectral hardness differences with statistical significance.
Findings
RLQ have higher X-ray luminosity than RQQ.
RLQ exhibit flatter (harder) X-ray spectra than RQQ.
Statistical tests confirm significant spectral differences.
Abstract
We performed a study of high redshift () quasars, looking for the main differences between Radio Loud Quasars (RLQ) and Radio Quiet Quasars (RQQ) in the X-ray band. Our sample of 472 RQQ and 81 RLQ was selected by cross-matching the SDSS DR7 quasars catalog with the Chandra Source Catalog. We computed the X-ray luminosity for the two samples and confirmed the X-ray luminosity excess of RLQ over RQQ. We fit the X-ray spectra assuming the absorbed power law model and obtained the photon index () values for all the sources in the sample. We excluded quasars with a low number of counts () and large uncertainty on the best-fit photon index (), and obtained the mean values of and for the RLQ and RQQ samples, respectively, showing that the RLQ have flatter…
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