Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Reionization, Redshift, and Metallicity.
A high black-hole-to-host mass ratio in a lensed AGN in the early Universe
Metal-poor star formation at <i>z</i> &gt; 6 with JWST: new insight into hard radiation fields and nitrogen enrichment on 20 pc scales
Lyα Emission Line Profiles of Extreme [O iii]- emitting Galaxies at z ≳ 2: Implications for Lyα Visibility in the Reionization Era
A <i>JWST</i>/NIRCam study of key contributors to reionization: the star-forming and ionizing properties of UV-faint <i>z</i> ∼ 7−8 galaxies
<i>JWST</i>/NIRSpec spectroscopy of <i>z</i> = 7–9 star-forming galaxies with CEERS: new insight into bright Lyα emitters in ionized bubbles
JWST UNCOVER: Extremely Red and Compact Object at z <sub>phot</sub> ≃ 7.6 Triply Imaged by A2744
Emission-line properties of IllustrisTNG galaxies: from local diagnostic diagrams to high-redshift predictions for <i>JWST</i>
Optical and mid-infrared line emission in nearby Seyfert galaxies
Detection of He++ ion in the star-forming ring of the Cartwheel using MUSE data and ionizing mechanisms
<scp>beagle</scp>-<scp>agn</scp> I: simultaneous constraints on the properties of gas in star-forming and AGN narrow-line regions in galaxies
Searching for Extremely Blue UV Continuum Slopes at z = 7–11 in JWST/NIRCam Imaging: Implications for Stellar Metallicity and Ionizing Photon Escape in Early Galaxies
The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas*
CLASSY. II. A Technical Overview of the COS Legacy Archive Spectroscopic Survey*
Direct Constraints on the Extremely Metal-poor Massive Stars Underlying Nebular C iv Emission from Ultra-deep HST/COS Ultraviolet Spectroscopy
A double-peaked Lyman-α emitter with a stronger blue peak multiply imaged by the galaxy cluster RXC J0018.5+1626
Constraints on the production and escape of ionizing radiation from the emission-line spectra of metal-poor star-forming galaxies