activity
20192026
most citedThe Host-Galaxy Properties of Type 1 Versus Type 2 Active Galactic Nuclei

73 citations · 162 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2025

VAR-PZ: Constraining the Photometric Redshifts of Quasars using Variability

S. Satheesh-Sheeba, R. J. Assef, T. Anguita +33

The Vera C. Rubin Observatory LSST is expected to discover tens of millions of new Active Galactic Nuclei (AGNs). The survey's exceptional cadence and sensitivity will enable UV/op…

astro-ph.GA2025

The Nature of an Unidentified X-ray Source in the 7 Ms Chandra Deep Field-South Catalog

Quinn P. Sullivan, Zhibo Yu, William N. Brandt +2

In the 7 Ms Chandra Deep Field-South catalog, only one source, XID 912, was highly significantly detected in X-rays but had no formally reported counterparts in the UV, optical, in…

astro-ph.GA2024

Investigating the Star-Formation Characteristics of Radio Active Galactic Nuclei

Bojun Zhang, Fan Zou, W. N. Brandt +5

The coevolution of supermassive black holes and their host galaxies represents a fundamental question in astrophysics. One approach to investigating this question involves comparin…

astro-ph.GA2024

A Rapidly Accreting Active Galactic Nucleus Hidden in a Dust-Obscured Galaxy at

Nathan Cristello, Fan Zou, William N. Brandt +3

Dust-obscured galaxies (DOGs) containing central supermassive black holes (SMBHs) that are rapidly accreting (i.e., having high Eddington ratios, ) may represent a…

astro-ph.GA2024

Dust-Obscured Galaxies in the XMM-SERVS Fields: Selection, Multiwavelength Characterization, and Physical Nature

Zhibo Yu, W. N. Brandt, Fan Zou +7

Dust-obscured galaxies (DOGs) are enshrouded by dust, and many are believed to host accreting supermassive black holes (SMBHs), which makes them unique objects for probing the coev…

astro-ph.GA2024

The Cosmic Evolution of the Supermassive Black Hole Population: A Hybrid Observed Accretion and Simulated Mergers Approach

Fan Zou, W. N. Brandt, Elena Gallo +4

Supermassive black holes (SMBHs) can grow through both accretion and mergers. It is still unclear how SMBHs evolve under these two channels from high redshifts to the SMBH populati…