Area of research
Instrumentation · Astronomy and Astrophysics
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Star formation.
Probing the star formation main sequence down to 10 <sup>7</sup> <i>M</i> <sub>⊙</sub> at 1 < <i>z</i> < 9
The Cosmic Evolution Early Release Science Survey (CEERS)
Improving Photometric Redshifts of Epoch of Reionization Galaxies: A New Empirical Transmission Curve with Neutral Hydrogen Damping Wing Ly<i>α</i> Absorption
Extreme properties of a compact and massive accreting black hole host in the first 500 Myr
CANUCS/Technicolor Data Release 1: Imaging, Photometry, Slit Spectroscopy, and Stellar Population Parameters*
Metal-poor Star-forming Clumps in Cosmic Noon Galaxies: Evidence for Gas Inflow and Chemical Dilution Using JWST NIRISS
Resolved Mass Assembly and Star Formation in Milky Way Progenitors since <i>z</i> = 5 from JWST/CANUCS: From Clumps and Mergers to Well-ordered Disks
The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ∼ 8.5–14.5
Outshining by Recent Star Formation Prevents the Accurate Measurement of High-z Galaxy Stellar Masses
Formation of a low-mass galaxy from star clusters in a 600-million-year-old Universe
ΛCDM not dead yet: massive high-<i>z</i> Balmer break galaxies are less common than previously reported
Evidence for a Shallow Evolution in the Volume Densities of Massive Galaxies at z = 4–8 from CEERS
Star Formation at the Epoch of Reionization with CANUCS: The Ages of Stellar Populations in MACS1149-JD1
The Ultraviolet Luminosity Function at 0.6 < z < 1 from UVCANDELS
CANUCS: UV and ionizing properties of dwarf star-forming galaxies at <i>z</i> ~ 5–7
When, where, and how star formation happens in a galaxy pair at cosmic noon using CANUCS <i>JWST</i>/NIRISS grism spectroscopy
The Firefly Sparkle: The Earliest Stages of the Assembly of A Milky Way-type Galaxy in a 600 Myr Old Universe
The FENIKS Survey: Multiwavelength Photometric Catalog in the UDS Field, and Catalogs of Photometric Redshifts and Stellar Population Properties
The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques
CEERS Spectroscopic Confirmation of NIRCam-selected z ≳ 8 Galaxy Candidates with JWST/NIRSpec: Initial Characterization of Their Properties
CEERS Key Paper. III. The Diversity of Galaxy Structure and Morphology at z = 3–9 with JWST
Dusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations
An Extremely Compact, Low-mass Galaxy on its Way to Quiescence at z = 5.2
A Milky Way-like barred spiral galaxy at a redshift of 3
Bursty star formation and galaxy–galaxy interactions in low-mass galaxies 1 Gyr after the Big Bang
CEERS Key Paper. II. A First Look at the Resolved Host Properties of AGN at 3 < z < 5 with JWST
Optimized Photometric Redshifts for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS)
The first large catalogue of spectroscopic redshifts in Webb’s first deep field, SMACS J0723.3−7327
Spectroscopy from Photometry: A Population of Extreme Emission Line Galaxies at 1.7 ≲ z ≲ 6.7 Selected with JWST Medium Band Filters
<i>JWST</i> catches the assembly of a <i>z</i> ∼ 5 ultra-low-mass galaxy