activity
20022024
most citedThe Chandra Deep Field-South Survey: 4 Ms Source Catalogs

581 citations · 9.1k across the 132 of their papers we have counts for

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Showing 2020Show all

9 papers · 1 filter

astro-ph.GA2020★ 14 cited

The environmental dependence of X-ray AGN activity at

E. Noordeh, R. E. A. Canning, A. King +9

We present an analysis of the X-ray Active Galactic Nucleus (AGN) population in a sample of seven massive galaxy clusters in the redshift range . We utilize high-quali…

astro-ph.HE2020★ 42 cited

The frequency of extreme X-ray variability of radio-quiet quasars

John D. Timlin, W. Niel Brandt, Shifu Zhu +3

We analyze 1598 serendipitous Chandra X-ray observations of 462 radio-quiet quasars to constrain the frequency of extreme amplitude X-ray variability that is intrinsic to the quasa…

astro-ph.GA2020★ 17 cited

Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-Triggered AGN-Galaxy Coevolution Models?

Junyao Li, Yongquan Xue, Mouyuan Sun +12

By using a large highly obscured () AGN sample (294 sources at ) selected from detailed X-ray spectral analyses in the deepest Chandra…

astro-ph.GA2020★ 1 cited

On the Fraction of X-ray Weak Quasars from the Sloan Digital Sky Survey

Xingting Pu, B. Luo, W. N. Brandt +4

We investigate systematically the X-ray emission from type 1 quasars using a sample of 1825 Sloan Digital Sky Survey (SDSS) non-broad absorption line (non-BAL) quasars with Chandra…

astro-ph.GA2020★ 42 cited

Revealing the relation between black-hole growth and host-galaxy compactness among star-forming galaxies

Q. Ni, W. N. Brandt, G. Yang +8

Recent studies show that a universal relation between black-hole (BH) growth and stellar mass () or star formation rate (SFR) is an oversimplification of BH-galaxy co-e…

astro-ph.HE2020★ 64 cited

The -- relation and corona-disk-jet connection in optically selected radio-loud quasars

S. F. Zhu, W. N. Brandt, B. Luo +3

Radio-loud quasars (RLQs) are more X-ray luminous than predicted by the X-ray-optical/UV relation (i.e. ) for radio-quiet quasars (RQQs). The e…