Chandra Detection of Three X-Ray Bright Quasars at z > 5-Reference-Cited by-同舟云学术

Chandra Detection of Three X-Ray Bright Quasars at z > 5

Published:2021-01-18 Issue:2 Volume:906 Page:135
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Li Jiang-Tao^ORCID,Wang Feige^ORCID,Yang Jinyi^ORCID,Zhang Yuchen,Fu Yuming^ORCID,Bian Fuyan^ORCID,Bregman Joel N.^ORCID,Fan Xiaohui^ORCID,Li Qiong^ORCID,Wu Xue-Bing^ORCID,Yu Xiaodi

Funder

National Aeronautics and Space Administration

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abc750/pdf

Reference42 articles.

1. X-Ray Constraints on the Spectral Energy Distribution of the z = 5.18 Blazar SDSS J013127.34−032100.1

2. An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5

3. The first blazar observed at z > 6

4. BLACK HOLE MASS ESTIMATES AND EMISSION-LINE PROPERTIES OF A SAMPLE OF REDSHIFTz> 6.5 QUASARS

5. Scaling variability from stellar to supermassive black holes

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1. A Strong He ii λ1640 Emitter with an Extremely Blue UV Spectral Slope at z = 8.16: Presence of Population III Stars?;The Astrophysical Journal Letters;2024-05-31

2. Is the X-ray bright z = 5.5 quasar SRGE J170245.3+130104 a blazar?;Monthly Notices of the Royal Astronomical Society;2022-12-22

3. Minute-timescale Variability in the X-ray Emission of the Highest Redshift Blazar*;The Astrophysical Journal;2021-10-01

4. A Chandra survey of z ≥ 4.5 quasars;Monthly Notices of the Royal Astronomical Society;2021-04-15

5. Discovery of the Most X-ray Luminous Quasar SRGE J170245.3+130104 at Redshift $$\boldsymbol{z\approx 5.5}$$;Astronomy Letters;2021-03