Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astrophysical Phenomena and Observations, Astronomy and Astrophysical Research, and Gamma-ray bursts and supernovae.
C <scp>iv</scp> wind properties of the SDSS-V X-ray selected quasars: strong optical-to-UV emission is key regardless of X-ray strength
<scp>Trinity</scp> – III. Quasar luminosity functions decomposed by halo, galaxy, and black hole masses as well as Eddington ratios from <i>z</i> = 0–10
<scp>Trinity</scp> IV: predictions for supermassive black holes at <i>z</i> ≳ 6
Hidden Little Monsters: Spectroscopic Identification of Low-mass, Broad-line AGNs at z > 5 with CEERS
<scp>Trinity</scp> II: The luminosity-dependent bias of the supermassive black hole mass–galaxy mass relation for bright quasars at z = 6
<scp>Trinity</scp> I: self-consistently modelling the dark matter halo–galaxy–supermassive black hole connection from <i>z</i> = 0–10
Athena synergies in the multi-messenger and transient universe
Supermassive black holes in cosmological simulations – II: the AGN population and predictions for upcoming X-ray missions
4MOST: Project overview and information for the First Call for Proposals
X-rays across the galaxy population – III. The incidence of AGN as a function of star formation rate
Deep ugrizY imaging and DEEP2/3 spectroscopy: a photometric redshift testbed for LSST and public release of data from the DEEP3 Galaxy Redshift Survey
X-rays across the galaxy population – II. The distribution of AGN accretion rates as a function of stellar mass and redshift
The evolution of the hard X-ray luminosity function of AGN
2016cited by 222position: first
X-rays across the galaxy population – I. Tracing the main sequence of star formation
PRIMUS + DEEP2: CLUSTERING OF X-RAY, RADIO, AND IR-AGNs AT z ∼ 0.7
The evolution of the X-ray luminosity functions of unabsorbed and absorbed AGNs out to z∼ 5
AEGIS-X: DEEP <i>CHANDRA</i> IMAGING OF THE CENTRAL GROTH STRIP
PRIMUS: THE RELATIONSHIP BETWEEN STAR FORMATION AND AGN ACCRETION
The X-ray luminosity function of active galactic nuclei in the redshift interval<i>z</i>=3-5
PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2 &lt; z &lt; 1
eScholarship (California Digital Library) 2014cited by 41position: middle
Investigating evidence for different black hole accretion modes since redshift z ∼ 1
Higher prevalence of X-ray selected AGN in intermediate-age galaxies up to z ∼ 1
PRIMUS: CONSTRAINTS ON STAR FORMATION QUENCHING AND GALAXY MERGING, AND THE EVOLUTION OF THE STELLAR MASS FUNCTION FROM<i>z</i>= 0-1
PRIMUS: INFRARED AND X-RAY AGN SELECTION TECHNIQUES AT 0.2 <<i>z</i>< 1.2
PRIMUS: AN OBSERVATIONALLY MOTIVATED MODEL TO CONNECT THE EVOLUTION OF THE ACTIVE GALACTIC NUCLEUS AND GALAXY POPULATIONS OUT TO<i>z</i>∼ 1
PRIMUS: THE DEPENDENCE OF AGN ACCRETION ON HOST STELLAR MASS AND COLOR