Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Reionization.
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
The Cosmic Evolution Early Release Science Survey (CEERS)
Galaxy mergers in the epoch of reionization – I. A JWST study of pair fractions, merger rates, and stellar mass accretion rates at <i>z</i> = 4.5–11.5
The evolution of [O <scp>iii</scp>] + Hβ equivalent width from <i>z</i> ≃ 3−8: implications for the production and escape of ionizing photons during reionization
Primordial rotating disk composed of at least 15 dense star-forming clumps at cosmic dawn
COSMOS2025: The COSMOS-Web galaxy catalog of photometry, morphology, redshifts, and physical parameters from JWST, HST, and ground-based imaging
Anatomy of a <i>z</i> = 6 Lyman-<i>α</i> emitter down to parsec scales
EPOCHS. I. The Discovery and Star-forming Properties of Galaxies in the Epoch of Reionization at 6.5 < <i>z</i> < 18 with PEARLS and Public JWST Data
Identification of more than 40 gravitationally magnified stars in a galaxy at redshift 0.725
EPOCHS paper – X. Environmental effects on Galaxy formation and protocluster Galaxy candidates at 4.5 &lt; <i>z</i> &lt; 10 from JWST observations
EPOCHS. XI. The Structure and Morphology of Galaxies in the Epoch of Reionization to <i>z</i> ∼ 12.5
Medium-band Astrophysics with the Grism of NIRCam In Frontier Fields (MAGNIF): Spectroscopic Census of H<i>α</i> Luminosity Functions and Cosmic Star Formation at <i>z</i> ∼ 4.5 and 6.3
Cosmology with supernova Encore in the strong lensing cluster MACS J0138−2155
Time-scales for the effects of interactions on galaxy properties and SMBH growth
The Intracluster Light Analysis of the Most Evolved Systems of Galaxies: Fossil Groups
Globular Clusters in the Galaxy Cluster MACS0416 at <i>z</i> = 0.397
The SDSS-V Black Hole Mapper Reverberation Mapping Project: Light Echoes of the Coronal-line Region in a Luminous Quasar
The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5–14.5
COSMOS-Web: Intrinsically Luminous z ≳ 10 Galaxy Candidates Test Early Stellar Mass Assembly
EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 < z < 13.5 Using 180 arcmin<sup>2</sup> of Deep, Blank Fields from the PEARLS Survey and Public JWST Data
The <i>JWST</i> EXCELS survey: too much, too young, too fast? Ultra-massive quiescent galaxies at 3 &lt; z &lt; 5
The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0
The evolution of star formation histories of quiescent galaxies
A luminous and young galaxy at z = 12.33 revealed by a JWST/MIRI detection of Hα and [O iii]
Deciphering Lyman-α emission deep into the epoch of reionization
Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy
On the Nature of Disks at High Redshift Seen by JWST/CEERS with Contrastive Learning and Cosmological Simulations
Efficient NIRCam Selection of Quiescent Galaxies at 3 < z < 6 in CEERS
Strong gravitational lensing’s ‘external shear’ is not shear
JWST Photometric Time-delay and Magnification Measurements for the Triply Imaged Type Ia “SN H0pe” at z = 1.78