# overview
I am a multiwavelength observational astrophysicist, and my research interests are broadly related to the ways that galaxies form (or don't form) new stars throughout the history of the Universe. I'm working on a number of topics related to the quenching of galaxies, trying to understand the physical mechanisms that turn a star-forming galaxy into a quiescent one.

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Kinematic Analysis of z = 4.3 Galaxies in the SPT234956 Protocluster Core

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The ramp-up of interstellar medium enrichment at z > 4

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Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo

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The Compact Structures of Massive z 0.7 Post-starburst Galaxies in the SQuIGG(L)over-right-arrowE Sample

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TEMPLATES: Direct Abundance Constraints for Two Lensed Lyman-break Galaxies

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Spatial variations in aromatic hydrocarbon emission in a dust-rich galaxy

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Constraining the Volume Density of Dusty Star-forming Galaxies through the First 3 mm Number Counts from ALMA

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Rejuvenation in z  0.8 Quiescent Galaxies in LEGA-C

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Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies

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ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z  1.5

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The ISM in the z=6.9 Interacting Galaxies of SPT0311-58

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Early Science with the Large Millimeter Telescope: Constraining the Gas Fraction of a Compact Quiescent Galaxy at z = 1.883

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The Rest-Frame Submillimeter Spectrum of High Redshift, Dusty, Star-Forming Galaxies from the SPT-SZ Survey

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ALMA Imaging and Gravitational Lens Models of South Pole Telescope-Selected Dusty, Star-Forming Galaxies at High Redshifts

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Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies. I. Sample Overview and Clumpy Structure in Molecular Outflows on 500 pc Scales

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Merger Signatures are Common, but not Universal, in Massive, Recently Quenched Galaxies at z  0.7

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LOW GAS FRACTIONS CONNECT COMPACT STAR-FORMING GALAXIES TO THEIR z  2 QUIESCENT DESCENDANTS

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The Complete Redshift Distribution of Dusty Star-forming Galaxies from the SPT-SZ Survey

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Stellar and Molecular Gas Rotation in a Recently Quenched Massive Galaxy at z  0.7

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On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z  2.0-2.5

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Star Formation Suppression by Tidal Removal of Cold Molecular Gas from an Intermediate-redshift Massive Post-starburst Galaxy

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ALMA Observations of the Sub-kpc Structure of the Host Galaxy of a z = 6.5 Lensed Quasar: A Rotationally Supported Hyper-Starburst System at the Epoch of Reionization

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Evidence for a Buried AGN in an Extremely Bright Dusty Galaxy at z = 2

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Erratum: The Brightest Galaxies in the Dark Ages: Galaxies Dust Continuum Emission during the Reionization Era (2018, ApJ, 862, 77)

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Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies II. Momentum-Driven Winds Powered by Star Formation in the Early Universe

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Searching Far and Long. I. Pilot ALMA 2 mm Follow-up of Bright Dusty Galaxies as a Redshift Filter

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Imaging the molecular interstellar medium in a gravitationally lensed star-forming galaxy at z = 5.7

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Star Formation Suppresion by Tidal Removal of Cold Molecular Gas from an Intermediate-Redshift Massive Post-Starburst Galaxy

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Spatially Resolved [C ii] Emission in SPT0346-52: A Hyper-starburst Galaxy Merger at z  5.7

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Molecular Gas Contents and Scaling Relations for Massive Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey

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Evidence for Inside-out Galaxy Growth and Quenching of a z  2 Compact Galaxy From High-resolution Molecular Gas Imaging

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1D Kinematics from Stars and Ionized Gas at z  0.8 from the LEGA-C Spectroscopic Survey of Massive Galaxies

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DESI Massive Poststarburst Galaxies at z  1.2 Have Compact Structures and Dense Cores

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Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies. II. Momentum-driven Winds Powered by Star Formation in the Early Universe

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Science with an ngVLA: Characterizing Feedback Through Molecular   Outflows Across Cosmic Time

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The Physical Drivers of the Luminosity-weighted Dust Temperatures in High-redshift Galaxies

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Brightest Cluster Galaxy Formation in the z=4.3 Protocluster SPT 2349-56: Discovery of a Radio-loud Active Galactic Nucleus

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ALMA 1.1 mm Observations of a Conservative Sample of High-redshift Massive Quiescent Galaxies in SHELA

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The Brightest Galaxies in the Dark Ages: Galaxies Dust Continuum Emission during the Reionization Era

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High-Redshift Extragalactic Science with the Single Aperture Large   Telescope for Universe Studies (SALTUS) Space Observatory

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REQUIEM-2D: A Diversity of Formation Pathways in a Sample of Spatially Resolved Massive Quiescent Galaxies at z  2

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The Rest-frame Submillimeter Spectrum of High-redshift, Dusty, Star-forming Galaxies from the SPT-SZ Survey

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Erratum:  SQuIGGLE : Studying Quenching in Intermediate-z Galaxies Gas, AnguLar Momentum, and Evolution (2022, ApJ, 926, 89)

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Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies I. Sample Overview and Clumpy Structure in Molecular Outflows on 500pc Scales

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TEMPLATES: Characterization of a Merger in the Dusty Lensing SPT041847 System

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Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-era Halo

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Source Structure and Molecular Gas Properties from High-resolution CO Imaging of SPT-selected Dusty Star-forming Galaxies

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Low Gas Fractions Connect Compact Star-Forming Galaxies to their z ~ 2 Quiescent Descendants

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Fast molecular outflow from a dusty star-forming galaxy in the early Universe.

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American Association for the Advancement of Science (AAAS)

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Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star-forming Galaxies at z  3

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The ALMA-CRISTAL Survey: Spatially Resolved Star Formation Activity and Dust Content in 4 < z < 6 Star-forming Galaxies

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Fast Molecular Outflow from a Dusty Star-Forming Galaxy in the Early Universe

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Centrally Concentrated Dust Emission in z  2 Compact Star-forming Galaxies

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High Molecular-gas to Dust Mass Ratios Predicted in Most Quiescent Galaxies

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Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies

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Massive Quenched Galaxies at z  0.7 Retain Large Molecular Gas Reservoirs

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Does the Lockstep Growth between Black Holes and Bulges Create Their Mass Relation?

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Spatial variations in aromatic hydrocarbon emission in a dust-rich galaxy.

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Detection of Intrinsic Source Structure at 3 Schwarzschild Radii with Millimeter-VLBI Observations of SAGITTARIUS A*

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JWST's TEMPLATES for Star Formation: The First Resolved Gas-phase Metallicity Maps of Dust-obscured Star-forming Galaxies at z 4

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Probing Cold Gas in a Massive, Compact Star-forming Galaxy at z=6

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The Role of Active Galactic Nuclei in the Quenching of Massive Galaxies in the SQuIGG E Survey

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Recovering the Star Formation Histories of Recently Quenched Galaxies: The Impact of Model and Prior Choices

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Multiphase ISM in the z = 5.7 Hyperluminous Starburst SPT 034652

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Molecular Line Observations in Two Dusty Star-forming Galaxies at z = 6.9

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Evidence for Inside-Out Galaxy Growth and Quenching of a z~2 Compact Galaxy from High-Resolution Molecular Gas Imaging

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Galactic outflows at high spatial resolution via gravitational lensing

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The Large Early Galaxy Astrophysics Census (LEGA-C) Data Release 2: Dynamical and Stellar Population Properties of z  1 Galaxies in the COSMOS Field

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Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z = 1.522

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Medium Bands, Mega Science: A JWST/NIRCam Medium-band Imaging Survey of A2744

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ALMA Measures Molecular Gas Reservoirs Comparable to Field Galaxies in a Low-mass Galaxy Cluster at z=1.3

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Sub-kiloparsec Imaging of Cool Molecular Gas in Two Strongly Lensed Dusty, Star-Forming Galaxies

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An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies

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Discovery of a Dark, Massive, ALMA-only Galaxy at z  56 in a Tiny 3 mm Survey

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Molecular Gas Reservoirs in Massive Quiescent Galaxies at z 0.7 Linked to Late-time Star Formation

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SQuIGGLE : Studying Quenching in Intermediate-z GalaxiesGas, AnguLar Momentum, and Evolution

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Comprehensive Gas Characterization of a z = 2.5 Protocluster: A Cluster Core Caught in the Beginning of Virialization?

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Extended Lyman- emission towards the SPT2349-56 protocluster at z = 4.3

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SQuIGG E Survey: Massive z  0.6 Post-starburst Galaxies Exhibit Flat Age Gradients

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Stellar Populations of over 1000 z  0.8 Galaxies from LEGA-C: Ages and Star Formation Histories from Dn4000 and H

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Now You See It, Now You Don't: Star Formation Truncation Precedes the Loss of Molecular Gas by 100 Myr in Massive Poststarburst Galaxies at z 0.6

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Molecular Gas Contents and Scaling Relations for Massive, Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey