activity
20092024
most citedGOODS-Herschel: The far-infrared view of star formation in AGN host galaxies since z~3

256 citations · 1.6k across the 18 of their papers we have counts for

collaborators

18 papers

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.HE2024

The X-ray enhancements of radio-loud quasars at high redshift: New results at

Zihao Zuo, Shifu Zhu, W. N. Brandt +4

Highly radio-loud quasars (HRLQs; ) at show apparent enhanced X-ray emission compared to matched HRLQs at lower redshifts, perhaps due to a redshift-depend…

astro-ph.GA2024★ 1 cited

High-quality Extragalactic Legacy-field Monitoring (HELM) with DECam

Ming-Yang Zhuang, Qian Yang, Yue Shen +45

High-quality Extragalactic Legacy-field Monitoring (HELM) is a long-term observing program that photometrically monitors several well-studied extragalactic legacy fields with the D…

astro-ph.GA2024★ 50 cited

Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results

Grisha Zeltyn, Benny Trakhtenbrot, Michael Eracleous +32

"Changing-look" active galactic nuclei (CL-AGNs) challenge our basic ideas about the physics of accretion flows and circumnuclear gas around supermassive black holes. Using first-y…

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.GA2017★ 109 cited

Linking black-hole growth with host galaxies: The accretion-stellar mass relation and its cosmic evolution

G. Yang, W. N. Brandt, F. Vito +9

Previous studies suggest that the growth of supermassive black holes (SMBHs) may be fundamentally related to host-galaxy stellar mass (). To investigate this SMBH growth-$…

astro-ph.GA2017★ 97 cited

X-ray spectral analyses of AGNs from the 7Ms Chandra Deep Field-South survey: the distribution, variability, and evolution of AGN's obscuration

Teng Liu, Paolo Tozzi, Jun-Xian Wang +18

We present a detailed spectral analysis of the brightest Active Galactic Nuclei (AGN) identified in the 7Ms Chandra Deep Field South (CDF-S) survey over a time span of 16 years. Us…

astro-ph.HE2017★ 91 cited

A New, Faint Population of X-ray Transients

F. E. Bauer, E. Treister, K. Schawinski +22

We report on the detection of a remarkable new fast high-energy transient found in the Chandra Deep Field-South, robustly associated with a faint ( mag, $z_{\rm ph}…

astro-ph.GA2015★ 82 cited

Mid-infrared luminous quasars in the GOODS-Herschel fields: a large population of heavily-obscured, Compton-thick quasars at z~2

A. Del Moro, D. M. Alexander, F. E. Bauer +10

We present the infrared (IR) and X-ray properties of a sample of 33 mid-IR luminous quasars (L(6 micron)>6x10 erg/s) at redshift z~1-3, identified through detailed spectr…

astro-ph.GA2014★ 34 cited

Photometric Redshifts in the Hawaii-Hubble Deep Field-North (H-HDF-N)

G. Yang, Y. Q. Xue, B. Luo +11

We derive photometric redshifts (\zp) for sources in the entire ( deg) Hawaii-Hubble Deep Field-North (\hdfn) field with the EAzY code, based on point spread function-…

astro-ph.CO2012★ 40 cited

The sub-mJy radio population of the E-CDFS: optical and infrared counterpart identification

M. Bonzini, V. Mainieri, P. Padovani +9

We study a sample of 883 sources detected in a deep Very Large Array survey at 1.4 GHz in the Extended Chandra Deep Field South. The paper focuses on the identification of their op…

astro-ph.CO2012★ 223 cited

The 4 Ms Chandra Deep Field-South Number Counts Apportioned by Source Class: Pervasive Active Galactic Nuclei and the Ascent of Normal Galaxies

B. D. Lehmer, Y. Q. Xue, W. N. Brandt +13

We present 0.5-2 keV, 2-8 keV, 4-8 keV, and 0.5-8 keV cumulative and differential number counts (logN-logS) measurements for the recently completed ~4 Ms Chandra Deep Field-South (…

astro-ph.CO2011★ 39 cited

The Radio - X-ray relation as a star formation indicator: Results from the VLA--E-CDFS Survey

S. Vattakunnel, P. Tozzi, F. Matteucci +10

In order to trace the instantaneous star formation rate at high redshift, and hence help understanding the relation between the different emission mechanisms related to star format…

astro-ph.CO2011★ 256 cited

GOODS-Herschel: The far-infrared view of star formation in AGN host galaxies since z~3

J. R. Mullaney, M. Pannella, E. Daddi +28

We present a study of the infrared properties of X-ray selected, moderate luminosity (Lx=10^{42}-10^{44}ergs/s) active galactic nuclei (AGNs) up to z~3, to explore the links betwee…

astro-ph.CO2011★ 142 cited

The XMM Deep survey in the CDFS I. First results on heavily obscured AGN

A. Comastri, P. Ranalli, K. Iwasawa +25

We present the first results of the spectroscopy of distant, obscured AGN as obtained with the ultra-deep (~3.3 Ms) XMM-Newton survey in the Chandra Deep Field South (CDFS). One of…

astro-ph.CO2010★ 28 cited

Radiation pressure, absorption and AGN feedback in the Chandra Deep Fields

S. I. Raimundo, A. C. Fabian, F. E. Bauer +5

The presence of absorbing gas around the central engine of Active Galactic Nuclei (AGN) is a common feature of these objects. Recent work has looked at the effect of the dust compo…

astro-ph.CO2010★ 232 cited

The LABOCA survey of the Extended Chandra Deep Field South: A photometric redshift survey of submillimetre galaxies

J. L. Wardlow, Ian Smail, K. E. K. Coppin +23

[abridged] We derive photometric redshifts from 17-band optical to mid-IR photometry of 74 robust counterparts to 68 of the 126 submillimetre galaxies (SMGs) selected at 870um by L…

astro-ph.CO2009★ 153 cited

BLAST: the far-infrared/radio correlation in distant galaxies

R. J. Ivison, David M. Alexander, Andy D. Biggs +32

We investigate the correlation between far-infrared (FIR) and radio luminosities in distant galaxies, a lynchpin of modern astronomy. We use data from the Balloon-borne Large Apert…