2020/11/02 by Jiang-Tao Li, Feige Wang, Jinyi Yang +8 · 12 citations
Physics and Astronomy · #Astrophysical Phenomena and Observations #Astrophysics and Cosmic Phenomena #Cosmology #Flux (metallurgy) #Galaxies: Formation, Evolution, Phenomena #Luminosity #Photon #Quasar #Redshift #Spectral index #Spectral line #astro-ph.CO #astro-ph.HE
paper · pdf · doi:10.3847/1538-4357/abc750
published in The Astrophysical Journal 906(2), 135 (IOP Publishing) · 12 pages, 5 figures, 2 tables, accepted for publication by ApJ
arxiv created 2020/11/02 · openalex created_date 2020/11/09 · openalex publication_date 2021/01/01 · arxiv updated 2021/01/27 · openalex updated_date 2026/08/08
Abstract We report Chandra detection of three UV-bright radio-quiet quasars at z ≳ 5. We have collected a sufficient number of photons to extract an X-ray spectrum of each quasar to measure their basic X-ray properties, such as the X-ray flux, power-law photon index (Γ), and optical-to-X-ray spectral slope ( α OX ). J074749+115352 at z = 5.26 is the X-ray brightest radio-quiet quasar at z > 5. It may have a short timescale variation (on a timescale of ∼3800 s in the observer’s frame, or ∼600 s in the rest frame), which is, however, largely embedded in the statistical noise. We extract phase folded spectra of this quasar. There are two distinguishable states: a “high soft” state with an average X-ray flux ∼2.7 times the “low hard” state, and a significantly steeper X-ray spectral slope ( versus ). We also compare the three quasars detected in this paper to other quasar samples. We find that J074749+115352, with an SMBH mass of M SMBH ≈ 1.8 × 10 9 M ⊙ and an Eddington ratio of λ Edd ≈ 2.3, is extraordinarily X-ray bright. It has an average α OX = −1.46 ± 0.02 and a 2–10 keV bolometric correction factor of L bol / L 2–10 keV = 42.4 ± 5.8, both significantly depart from some well defined scaling relations. We compare Γ of the three quasars to other samples at different redshifts, and do not find any significant redshift evolution based on the limited sample of z > 5 quasars with reliable measurements of the X-ray spectral properties.