activity
20172026
most citedOn the Observational Difference Between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei

65 citations · 713 across the 40 of their papers we have counts for

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Showing astro-ph.GAShow all

34 papers · 1 filter

astro-ph.GA2026★ 2 cited

CIV wind properties of the SDSS-V X-ray selected quasars: strong optical-to-UV emission is key regardless of X-ray strength

Amy L. Rankine, David Homan, James Aird +25

We present an investigation of the rest-frame optical/UV and X-ray properties for a sample of 3027 X-ray selected quasars between detected in the deepest Spec…

astro-ph.GA2025

The Drivers of the Decline in Supermassive Black Hole Growth at

Zhibo Yu, W. N. Brandt, Fan Zou +4

It is well established that cosmic supermassive black hole (SMBH) growth peaks at , followed by a strong decline of toward the present day, w…

astro-ph.GA2025

On the Extremely X-ray Variable Active Galactic Nuclei in the XMM-LSS Field

Zijian Zhang, Bin Luo, Linhua Jiang +3

We present a systematic investigation of extremely X-ray variable active galactic nuclei (AGNs) in the XMM-SERVS XMM-LSS region. Eight variable AGNs are i…

astro-ph.GA2024★ 4 cited

Photometric Selection of type 1 Quasars in the XMM-LSS Field with Machine Learning and the Disk-Corona Connection

Jian Huang, Bin Luo, W. N. Brandt +4

We present photometric selection of type 1 quasars in the XMM-Large Scale Structure (XMM-LSS) survey field with machine learning. We constructed our trai…

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

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.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.GA2024★ 49 cited

The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles

Yi Zhang, Johan Comparat, Gabriele Ponti +17

The circumgalactic medium (CGM) provides the material needed for galaxy formation and influences galaxy evolution. The hot () CGM is poorly detected around galaxies with s…

astro-ph.GA2023★ 1 cited

The LSST AGN Data Challenge: Selection methods

Đorđe V. Savić, Isidora Jankov, Weixiang Yu +12

Development of the Rubin Observatory Legacy Survey of Space and Time (LSST) includes a series of Data Challenges (DC) arranged by various LSST Scientific Collaborations (SC) that a…

astro-ph.GA2023★ 12 cited

The incidence of AGN in galaxies with different stellar population ages

Q. Ni, J. Aird, A. Merloni +4

It has been argued that recycled gas from stellar mass loss in galaxies might serve as an important fuelling source for black holes (BHs) in their centers. Utilizing spectroscopic…

astro-ph.GA2023★ 17 cited

The relation of cosmic environment and morphology with the star formation and stellar populations of AGN and non-AGN galaxies

G. Mountrichas, G. Yang, V. Buat +5

In this work, we study the relation of cosmic environment and morphology with the star-formation (SF) and the stellar population of galaxies. Most importantly, we examine if this r…

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.GA2022★ 3 cited

Does the lockstep growth between black holes and bulges create their mass relation?

Guang Yang, W. N. Brandt, David M. Alexander +7

Recent studies have revealed a strong relation between sample-averaged black-hole (BH) accretion rate (BHAR) and star formation rate (SFR) among bulge-dominated galaxies, i.e., "lo…

astro-ph.GA2022★ 1 cited

Comparison of star formation histories of AGN and non-AGN galaxies

G. Mountrichas, V. Buat, G. Yang +6

We use AGN with , from the COSMOS-Legacy survey that lie within the UltraVISTA region and cross match them with the LEGA-C catalogue. The…

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.GA2022

A quasar shedding its dust cocoon at redshift 2

Weimin Yi, W. N. Brandt, Q. Ni +12

We present the first near-IR spectroscopy and joint analyses of multi-wavelength observations for SDSS J082747.14+425241.1, a dust-reddened, weak broad emission-line quasar (WLQ) u…

astro-ph.GA2022★ 15 cited

Connecting Low- and High-Redshift Weak Emission-Line Quasars via HST Spectroscopy of Ly Emission

Jeremiah D. Paul, Richard M. Plotkin, Ohad Shemmer +10

We present ultraviolet spectroscopy covering the Ly + N V complex of six candidate low-redshift () weak emission-line quasars (WLQs) based on observations with th…

astro-ph.GA2022★ 33 cited

Sensitive Chandra coverage of a representative sample of weak-line quasars: revealing the full range of X-ray properties

Q. Ni, W. N. Brandt, B. Luo +8

We present deeper Chandra observations for weak-line quasars (WLQs) in a representative sample that previously had limited X-ray constraints, and perform X-ray photometric analyses…

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…