Richard Ellis
iris.ucl.ac.uk
0000-0001-7782-7071
University College London
28 papers found
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The Lyman Continuum Escape Survey. II. Ionizing Radiation as a Function of the [O iii]/[O ii] Line Ratio
The Dark Matter Distributions in Low-mass Disk Galaxies. II. The Inner Density Profiles
Evolution of the Stellar Mass–Metallicity Relation. II. Constraints on Galactic Outflows from the Mg Abundances of Quiescent Galaxies
The Lyman Continuum Escape Survey: Ionizing Radiation from [O iii]-strong Sources at a Redshift of 3.1
MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II. Star Formation Histories and Galaxy Quenching
The Dark Matter Distributions in Low-mass Disk Galaxies. I. Hα Observations Using the Palomar Cosmic Web Imager
Resolving Quiescent Galaxies at z ≳ 2. I. Search for Gravitationally Lensed Sources and Characterization of Their Structure, Stellar Populations, and Line Emission
Resolving Quiescent Galaxies at z ≳ 2. II. Direct Measures of Rotational Support
The Redshift Evolution of Rest-UV Spectroscopic Properties in Lyman-break Galaxies atz∼ 2–4
Evolution of the Stellar Mass–Metallicity Relation. I. Galaxies in thez∼ 0.4 Cluster Cl0024
Spectra of Hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory
A Spectroscopic Search for AGN Activity in the Reionization Era
Thez∼ 6 Luminosity Function Fainter than −15 mag from the Hubble Frontier Fields: The Impact of Magnification Uncertainties
High-resolution Velocity Fields of Low-mass Disk Galaxies. I. CO Observations
Dust in the Reionization Era: ALMA Observations of a z = 8.38 Gravitationally Lensed Galaxy
Mosfire Spectroscopy of Quiescent Galaxies at 1.5
Absorption-Line Spectroscopy of Gravitationally Lensed Galaxies: Further Constraints on the Escape Fraction of Ionizing Photons at High Redshift
A HARD IONIZING SPECTRUM IN Z = 3–4 Ly α EMITTERS WITH INTENSE $[{\Rm{O}}\,{\rm{III}}]$ EMISSION: ANALOGS OF GALAXIES IN THE REIONIZATION ERA?
DETECTION OF THREE GAMMA-RAY BURST HOST GALAXIES ATz∼ 6
Luminous and Dark Matter Profiles From Galaxies to Clusters: Bridging the Gap With Group-Scale Lenses
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