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

73 citations · 273 across the 20 of their papers we have counts for

collaborators

21 papers

astro-ph.GA2026

VAR-PZnn: A machine-learning framework for AGN photometric redshifts using color and variability-based features

S. Satheesh-Sheeba, P. Sánchez-Sáez, R. J. Assef +39

Photometric redshift estimation for active galactic nuclei (AGNs) remains a fundamental challenge for current and upcoming large-scale photometric surveys. Traditional spectral ene…

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…

astro-ph.HE2024

The Remarkable X-ray Spectra and Variability of the Ultraluminous Weak-Line Quasar SDSS J1521+5202

Shouyi Wang, W. Niel Brandt, Bin Luo +4

We present a focused X-ray and multiwavelength study of the ultraluminous weak-line quasar (WLQ) SDSS J1521+5202, one of the few X-ray weak WLQs that is amenable to basic X-ray spe…

astro-ph.GA2024★ 23 cited

Mapping the Growth of Supermassive Black Holes as a Function of Galaxy Stellar Mass and Redshift

Fan Zou, Zhibo Yu, W. N. Brandt +3

The growth of supermassive black holes is strongly linked to their galaxies. It has been shown that the population mean black-hole accretion rate () prima…

astro-ph.GA2024

Investigating the Star Formation Rates of AGN Hosts Relative to the Star-Forming Main Sequence

Nathan Cristello, Fan Zou, W. N. Brandt +4

A fundamental question in galaxy and black-hole evolution remains how galaxies and their supermassive black holes have evolved together over cosmic time. Specifically, it is still…

astro-ph.GA2023

Stellar Masses and Star-Formation Rates of Galaxies and AGNs in the eFEDS GAMA09 Field

Zhibo Yu, Fan Zou, William N. Brandt

The eFEDS is a wide 140 deg field that has extensive multiwavelength coverage. To improve the utility of the existing data, we use CIGALE to fit source Spectral Energ…

astro-ph.GA2023★ 15 cited

Radio AGN Selection and Characterization in Three Deep-Drilling Fields of the Vera C. Rubin Observatory Legacy Survey of Space and Time

Shifu Zhu, William N. Brandt, Fan Zou +4

The Australia Telescope Large Area Survey (ATLAS) and the VLA survey in the XMM-LSS/VIDEO deep field provide deep ( Jybeam) and high-resolution ( 4.5…

astro-ph.GA2023★ 13 cited

The Most Obscured AGNs in the XMM-SERVS Fields

Wei Yan, W. N. Brandt, Fan Zou +9

We perform X-ray spectral analyses to derive characteristics (e.g., column density, X-ray luminosity) of 10,200 active galactic nuclei (AGNs) in the XMM-Spitzer Extragalac…

astro-ph.GA2023★ 4 cited

Investigation of Stellar Kinematics and Ionized gas Outflows in Local (U)LIRGs

Ashraf Ayubinia, Yongquan Xue, Huynh Anh Nguyen Le +4

We explore properties of stellar kinematics and ionized gas in a sample of 1106 local (U)LIRGs from the AKARI telescope. We combine data from $Wide-field\ Infrared\ Survey\ Explore…

astro-ph.GA2022★ 8 cited

The Nature of Luminous Quasars with Very Large C IV Equivalent Widths

Shuqi Fu, W. N. Brandt, Fan Zou +5

We report results for a complete sample of ten luminous radio-quiet quasars with large C IV equivalent widths (EW > 150 A). For 8/10 we performed Chandra snapshot observations. We…

astro-ph.GA2022★ 47 cited

Spectral Energy Distributions in Three Deep-Drilling Fields of the Vera C. Rubin Observatory Legacy Survey of Space and Time: Source Classification and Galaxy Properties

Fan Zou, W. N. Brandt, Chien-Ting Chen +9

W-CDF-S, ELAIS-S1, and XMM-LSS will be three Deep-Drilling Fields (DDFs) of the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST), but their extensive multi-waveleng…

astro-ph.GA2021★ 46 cited

The XMM-SERVS survey: XMM-Newton point-source catalogs for the W-CDF-S and ELAIS-S1 fields

Q. Ni, W. N. Brandt, C. -T. Chen +30

We present the X-ray point-source catalogs in two of the XMM-Spitzer Extragalactic Representative Volume Survey (XMM-SERVS) fields, W-CDF-S (4.6 deg) and ELAIS-S1 (3.2 deg)…

astro-ph.GA2021★ 10 cited

Photometric Redshifts in the W-CDF-S and ELAIS-S1 Fields Based on Forced Photometry from 0.36 -- 4.5 Microns

Fan Zou, Guang Yang, W. N. Brandt +10

The W-CDF-S and ELAIS-S1 fields will be two of the LSST Deep Drilling fields, but the availability of spectroscopic redshifts within these two fields is still limited on deg^2 scal…

astro-ph.GA2021★ 10 cited

A Multi-Band Forced-Photometry Catalog in the ELAIS-S1 Field

Fan Zou, W. N. Brandt, Mark Lacy +11

The ELAIS-S1 field will be an LSST Deep Drilling field, and it also has extensive multiwavelength coverage. To improve the utility of the existing data, we use The Tractor to perfo…

astro-ph.GA2020★ 24 cited

Chandra reveals a luminous Compton-thick QSO powering a blob in a starbursting protocluster

Fabio Vito, William Nielsen Brandt, Bret Darby Lehmer +7

Galaxy clusters in the local universe descend from high-redshift overdense regions known as protoclusters. The large gas reservoirs and high rate of galaxy interaction in protoclus…

astro-ph.GA2019★ 73 cited

The Host-Galaxy Properties of Type 1 Versus Type 2 Active Galactic Nuclei

Fan Zou, Guang Yang, William N. Brandt +1

The unified model of active galactic nuclei (AGNs) proposes that different AGN optical spectral types are caused by different viewing angles with respect to an obscuring 'torus'. T…