Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Redshift, Astronomy, and Ionizing radiation.
A fully automated machine-learning-based workflow for radiation treatment planning in prostate cancer
The connection between the escape of ionizing radiation and galaxy properties at <i>z</i> ∼ 3 in the Keck Lyman continuum spectroscopic survey
A Glimpse of the Stellar Populations and Elemental Abundances of Gravitationally Lensed, Quiescent Galaxies at z ≳ 1 with Keck Deep Spectroscopy
The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas*
CLASSY III. The Properties of Starburst-driven Warm Ionized Outflows*
The Effects of Stellar Population and Gas Covering Fraction on the Emergent Lyα Emission of High-redshift Galaxies*
CLASSY. II. A Technical Overview of the COS Legacy Archive Spectroscopic Survey*
An uncontaminated measurement of the escaping Lyman continuum at<i>z</i>∼ 3
The MOSDEF Survey: The First Direct Measurements of the Nebular Dust Attenuation Curve at High Redshift*
The Keck Baryonic Structure Survey: using foreground/background galaxy pairs to trace the structure and kinematics of circumgalactic neutral hydrogen at <i>z</i> ∼ 2
Multi-filament gas inflows fuelling young star-forming galaxies
The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-redshift Galaxies
A comparison of observed and simulated absorption from H <scp>i</scp>, C <scp>iv</scp>, and Si <scp>iv</scp>around<i>z</i> ≈ 2 star-forming galaxies suggests redshift–space distortions are due to inflows
The evolution of the hard X-ray luminosity function of AGN
2016cited by 222position: middle
Q1549-C25: A CLEAN SOURCE OF LYMAN-CONTINUUM EMISSION AT z = 3.15<sup>∗</sup>
Testing metallicity indicators at z ∼ 1.4 with the gravitationally lensed galaxy CASSOWARY 20★
A REFINED ESTIMATE OF THE IONIZING EMISSIVITY FROM GALAXIES AT<i>z</i>≃ 3: SPECTROSCOPIC FOLLOW-UP IN THE SSA22a FIELD
THE COLUMN DENSITY DISTRIBUTION AND CONTINUUM OPACITY OF THE INTERGALACTIC AND CIRCUMGALACTIC MEDIUM AT REDSHIFT ⟨<i>z</i>⟩ = 2.4
THE MASS-METALLICITY RELATION OF A<i>z</i>∼ 2 PROTOCLUSTER WITH MOSFIRE
A measurement of galaxy halo mass from the surrounding H i Lyα absorption
MOSFIRE, the multi-object spectrometer for infra-red exploration at the Keck Observatory
THE CHARACTERISTIC STAR FORMATION HISTORIES OF GALAXIES AT REDSHIFTS<i>z</i>∼ 2-7
High velocity dispersion in a rare grand-design spiral galaxy at redshift z = 2.18