Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Astrophysics, Physics, Quasar, Redshift, Reionization, and Galaxy.
‘Little red dots’ cannot reside in the same dark matter haloes as comparably luminous unobscured quasars
A post-starburst pathway for the formation of massive galaxies and black holes at z > 6
A little red dot at z = 7.3 within a large galaxy overdensity
A SPectroscopic Survey of Biased Halos In the Reionization Era (ASPIRE): Broad-line AGN at z = 4−5 Revealed by JWST/NIRCam WFSS
A quasar-galaxy merger at <i>z</i> ∼ 6.2: Rapid host growth via the accretion of two massive satellite galaxies
A blazar in the epoch of reionization
A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): Impact of Galaxies on the Circumgalactic Medium Metal Enrichment at z > 6 Using the JWST and VLT
Detection of stellar light from quasar host galaxies at redshifts above 6
A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z = 6.61 Quasar
A SPectroscopic Survey of Biased Halos in the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of z > 6.5 Quasars Using JWST
The Pan-STARRS1 z > 5.6 Quasar Survey. II. Discovery of 55 Quasars at 5.6 < z < 6.5
XQR-30: Black hole masses and accretion rates of 42 <i>z</i> ≳ 6 quasars
The Pan-STARRS1 z > 5.6 Quasar Survey. III. The z ≈ 6 Quasar Luminosity Function
Hydrogen reionization ends by <i>z</i> = 5.3: Lyman-α optical depth measured by the XQR-30 sample
The X–shooter/ALMA Sample of Quasars in the Epoch of Reionization. II. Black Hole Masses, Eddington Ratios, and the Formation of the First Quasars
Suppression of black-hole growth by strong outflows at redshifts 5.8–6.6
Chemical abundance of <i>z</i> ~ 6 quasar broad-line regions in the XQR-30 sample
Probing Early Supermassive Black Hole Growth and Quasar Evolution with Near-infrared Spectroscopy of 37 Reionization-era Quasars at 6.3 < z ≤ 7.64
The Kinematics of z ≳ 6 Quasar Host Galaxies
Revealing the Accretion Physics of Supermassive Black Holes at Redshift z ∼ 7 with Chandra and Infrared Observations
The X-SHOOTER/ALMA Sample of Quasars in the Epoch of Reionization. I. NIR Spectral Modeling, Iron Enrichment, and Broad Emission Line Properties
Detecting and Characterizing Young Quasars. I. Systemic Redshifts and Proximity Zone Measurements
DSpace@MIT (Massachusetts Institute of Technology) 2020cited by 15position: middle
Filling in the Quasar Redshift Gap at z ∼ 5.5. II. A Complete Survey of Luminous Quasars in the Post-reionization Universe
The Discovery of a Luminous Broad Absorption Line Quasar at a Redshift of 7.02
The Extremely Luminous Quasar Survey in the Sloan Digital Sky Survey Footprint. II. The North Galactic Cap Sample
Quasar Photometric Redshifts and Candidate Selection: A New Algorithm Based on Optical and Mid-infrared Photometric Data
EXPLORING STELLAR EVOLUTION MODELS OF sdB STARS USING MESA