Publications

Rest-frame Near-infrared Sizes of Galaxies at Cosmic Noon: Objects in JWST's Mirror Are Smaller than They Appeared. apjl, 2022.
Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past. arXiv e-prints, 2022.
Euclid preparation. XXV. The Euclid Morphology Challenge -- Towards model-fitting photometry for billions of galaxies. arXiv e-prints, 2022.
Euclid preparation XXVI: The Euclid Morphology Challenge. Towards structural parameters for billions of galaxies. arXiv e-prints, 2022.
Early JWST imaging reveals strong optical and NIR color gradients in galaxies at $z∼2$ driven mostly by dust. arXiv e-prints, 2022.
Diagnosing deceivingly cold dusty galaxies at 3.5 < z < 6: A substantial population of compact starbursts with high infrared optical depths. åp, 2022.
COSMOS2020: Manifold learning to estimate physical parameters in large galaxy surveys. åp, 2022.
A galaxy group candidate at z ensuremath≈ 3.7 in the COSMOS field. åp, 2022.
Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z≈17$, or Dusty/Quenched at $z≈5$?. arXiv e-prints, 2022.
JWST reveals a population of ultra-red, flattened disk galaxies at 2<z<6 previously missed by HST. arXiv e-prints, 2022.
COSMOS2020: Cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z ensuremath∼ 5. åp, 2022.
A Machine Learning Approach to Predict Missing Flux Densities in Multi-band Galaxy Surveys. arXiv e-prints, 2022.
Unveiling the Nature of Infrared Bright, Optically Dark Galaxies with Early JWST Data. arXiv e-prints, 2022.
Two Remarkably Luminous Galaxy Candidates at $z≈11-13$ Revealed by JWST. arXiv e-prints, 2022.
Pilot-WINGS: An extended MUSE view of the structure of Abell 370. mnras, 2022.
Implications of a Temperature-dependent Initial Mass Function. III. Mass Growth and Quiescence. apj, 2022.
COSMOS2020: UV selected galaxies at $z≥7.5$. arXiv e-prints, 2022.
ALMA Lensing Cluster Survey: $HST$ and $Spitzer$ Photometry of 33 Lensed Fields Built with CHArGE. arXiv e-prints, 2022.
Implications of a Temperature-dependent Initial Mass Function. II. An Updated View of the Star-forming Main Sequence. apj, 2022.
Implications of a Temperature-dependent Initial Mass Function. I. Photometric Template Fitting. apj, 2022.
Euclid preparation: XXI. Intermediate-redshift contaminants in the search for $z>6$ galaxies within the Euclid Deep Survey. arXiv e-prints, 2022.
The Archival Discovery of a Strong Lyensuremathα and [C II] Emitter at z = 7.677. apjl, 2022.
Joint Survey Processing. I. Compact Oddballs in the COSMOS Field-Low-luminosity Quasars at z > 6?. apj, 2022.
COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at 0 < z < 5 Revealed by X-Ray and Radio Stacking. apj, 2022.
Euclid preparation. XVII. Cosmic Dawn Survey: Spitzer Space Telescope observations of the Euclid deep fields and calibration fields. åp, 2022.
COSMOS2020: A Panchromatic View of the Universe to z 10 from Two Complementary Catalogs. apjs, 2022.
Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies. apj, 2021.
Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters. apj, 2021.
The Evolving Interstellar Medium of Star-forming Galaxies, as Traced by Stardust. apj, 2021.
Euclid preparation: XVIII. Cosmic Dawn Survey. Spitzer observations of the Euclid deep fields and calibration fields. arXiv e-prints, 2021.
COSMOS2020: A panchromatic view of the Universe to $z∼10$ from two complementary catalogs. arXiv e-prints, 2021.
Joint Survey Processing I: Compact oddballs in the COSMOS field -- low-luminosity Quasars at z > 6?. arXiv e-prints, 2021.
Galaxy Protoclusters as Drivers of Cosmic Reionization. 2021.
Beasts in the Bubbles: Characterizing ultra-luminous galaxies at Cosmic Dawn. 2021.
COSMOS2020: A next-generation catalog to explore the 1 < z < 8 universe. American Astronomical Society Meeting Abstracts, 2021.
Comparison of stellar populations in simulated and real post-starburst galaxies in MaNGA. mnras, 2020.
The BUFFALO HST Survey. apjs, 2020.
A Method to Distinguish Quiescent and Dusty Star-forming Galaxies with Machine Learning. apj, 2020.
Improving star-galaxy seperation with neural networks. American Astronomical Society Meeting Abstracts #235, 2020.
Finding High Redshift Galaxies Using the 3D-HST Survey. American Astronomical Society Meeting Abstracts #235, 2020.
The Farmer: Improved model-based photometry for the next generation of galaxy surveys. The Art of Measuring Galaxy Physical Properties, 2019.
History and destiny of an emerging early-type galaxy. New IFU insights on the major-merger remnant NGC 7252. åp, 2018.
SpecDB: The AAVSOtextquoterights Public Repository for Spectra of Variable Stars. American Astronomical Society Meeting Abstracts #231, 2018.
Integral Field Spectroscopy of the Merger Remnant NGC 7252. American Astronomical Society Meeting Abstracts #231, 2018.
Searching for Extreme High Redshift Galaxies with HST Grism Spectroscopy. American Astronomical Society Meeting Abstracts #229, 2017.
A Survey of Localized Star Clusters in NGC 1427A. American Astronomical Society Meeting Abstracts #227, 2016.