Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Astrophysics and Cosmic Phenomena, and Astrophysical Phenomena and Observations.
The Black Hole Explorer: motivation and vision
The Black Hole Explorer: photon ring science, detection, and shape measurement
Brightest Cluster Galaxy Formation in the z = 4.3 Protocluster SPT 2349-56: Discovery of a Radio-loud Active Galactic Nucleus
SPT-SZ MCMF: an extension of the SPT-SZ catalogue over the DES region
Single Aperture Large Telescope for Universe Studies: science overview
Spatial variations in aromatic hydrocarbon emission in a dust-rich galaxy
The Rest-frame Submillimeter Spectrum of High-redshift, Dusty, Star-forming Galaxies from the SPT-SZ Survey
[C ii] Spectral Mapping of the Galactic Wind and Starbursting Disk of M82 with SOFIA
Millimeter Light Curves of Sagittarius A* Observed during the 2017 Event Horizon Telescope Campaign
CMB/kSZ and Compton-y Maps from 2500 deg<sup>2</sup> of SPT-SZ and Planck Survey Data
Selective Dynamical Imaging of Interferometric Data
SPT-SLIM: A Line Intensity Mapping Pathfinder for the South Pole Telescope
An Intensity Mapping Constraint on the CO-galaxy Cross-power Spectrum at Redshift ∼3
High resolution spectral imaging of CO(7–6), [CI](2–1), and continuum of three high-<i>z</i> lensed dusty star-forming galaxies using ALMA
Multiphase ISM in the z = 5.7 Hyperluminous Starburst SPT 0346–52
Molecular Line Observations in Two Dusty Star-forming Galaxies at z = 6.9
Overdensities of submillimetre-bright sources around candidate protocluster cores selected from the South Pole Telescope survey
Optical and near-infrared observations of the SPT2349-56 proto-cluster core at <i>z</i> = 4.3
Rapid build-up of the stellar content in the protocluster core SPT2349−56 at z = 4.3
The shape of the black hole photon ring: A precise test of strong-field general relativity
The Complete Redshift Distribution of Dusty Star-forming Galaxies from the SPT-SZ Survey
Megaparsec-scale structure around the protocluster core SPT2349–56 at <i>z</i> = 4.3
An Intensity Mapping Detection of Aggregate CO Line Emission at 3 mm
Ubiquitous Molecular Outflows in z &gt; 4 Massive, Dusty Galaxies. I. Sample Overview and Clumpy Structure in Molecular Outflows on 500 pc Scales
eScholarship (California Digital Library) 2020cited by 41position: middle
Ubiquitous Molecular Outflows in z &gt; 4 Massive, Dusty Galaxies. II. Momentum-driven Winds Powered by Star Formation in the Early Universe
eScholarship (California Digital Library) 2020cited by 41position: middle
The [C <scp>ii</scp>]/[N <scp>ii</scp>] ratio in 3 &lt; <i>z</i> &lt; 6 sub-millimetre galaxies from the South Pole Telescope survey
Biases and Cosmic Variance in Molecular Gas Abundance Measurements at High Redshift
The Size, Shape, and Scattering of Sagittarius A* at 86 GHz: First VLBI with ALMA
LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content
Constraints on the Thermal Contents of the X-Ray Cavities of Cluster MS 0735.6+7421 with Sunyaev–Zel’dovich Effect Observations
Collaborative Research: It's TIME! Mapping cosmic star formation history with CO and CII
MRI: Development of the Next Generation 211-373 GHz Receiver for the Arizona Radio Observatory’s Sub-mm Telescope
CAREER: Mapping the Fuel for Star Formation Across Cosmic History
Collaborative Research: Exploring Galaxy Evolution at High Resolution with Gravitational Lensing and ALMA
Exploring Galaxy Evolution and Missing Satellites with ALMA and Gravitational Lensing
Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole Telescope