| Testing Evolutionary Models with Red Supergiant and Wolf–Rayet Populations P Massey, KF Neugent, TZ Dorn-Wallenstein, JJ Eldridge, ER Stanway, ... The Astrophysical Journal 922 (2), 177, 2021 | 28 | 2021 |
| Stellar population diagnostics of the massive star binary fraction TZ Dorn-Wallenstein, EM Levesque The Astrophysical Journal 867 (2), 125, 2018 | 25 | 2018 |
| No strong geometric beaming in the ultraluminous neutron star binary NGC 300 ULX-1 (SN 2010da) from swift and gemini B Binder, EM Levesque, T Dorn-Wallenstein The Astrophysical Journal 863 (2), 141, 2018 | 25 | 2018 |
| Short-term variability of evolved massive stars with TESS. II. A new class of cool, pulsating supergiants TZ Dorn-Wallenstein, EM Levesque, KF Neugent, JRA Davenport, ... The Astrophysical Journal 902 (1), 24, 2020 | 22 | 2020 |
| A Mote in Andromeda's Disk: A Misidentified Periodic AGN behind M31 T Dorn-Wallenstein, EM Levesque, JJ Ruan The Astrophysical Journal 850 (1), 86, 2017 | 21 | 2017 |
| Short-term Variability of Evolved Massive Stars with TESS TZ Dorn-Wallenstein, EM Levesque, JRA Davenport The Astrophysical Journal 878 (2), 155, 2019 | 20 | 2019 |
| A Comparison of Rotating and Binary Stellar Evolution Models: Effects on Massive Star Populations TZ Dorn-Wallenstein, EM Levesque The Astrophysical Journal 896 (2), 164, 2020 | 14 | 2020 |
| Photometric detection of internal gravity waves in upper main-sequence stars-III. Comparison of amplitude spectrum fitting and Gaussian process regression using CELERITE2 DM Bowman, TZ Dorn-Wallenstein Astronomy & Astrophysics 668, A134, 2022 | 7 | 2022 |
| Photometric classifications of evolved massive stars: Preparing for the era of Webb and Roman with machine learning TZ Dorn-Wallenstein, JRA Davenport, D Huppenkothen, EM Levesque The Astrophysical Journal 913 (1), 32, 2021 | 7 | 2021 |
| The Properties of Fast Yellow Pulsating Supergiants: FYPS Point the Way to Missing Red Supergiants TZ Dorn-Wallenstein, EM Levesque, JRA Davenport, KF Neugent, ... The Astrophysical Journal 940 (1), 27, 2022 | 5 | 2022 |
| 13 yr of P Cygni Spectropolarimetry: Investigating Mass Loss through Hα, Periodicity, and Ellipticity K Gootkin, T Dorn-Wallenstein, JR Lomax, G Eadie, EM Levesque, ... The Astrophysical Journal 900 (2), 162, 2020 | 4 | 2020 |
| aesop: ARC Echelle Spectroscopic Observation Pipeline. BM Morris, T Dorn-Wallenstein J. Open Source Softw. 3 (28), 854, 2018 | 4 | 2018 |
| Photometric Metallicities for Low-mass Stars with Gaia and WISE JRA Davenport, TZ Dorn-Wallenstein Research Notes of the AAS 3 (3), 54, 2019 | 3 | 2019 |
| Physical Properties of 5000 Cool Large Magellanic Cloud Supergiants with Gaia XP Spectra: A Detailed Portrait of the Upper HR Diagram Hints at Missing Supernova Progenitors TZ Dorn-Wallenstein, KF Neugent, EM Levesque The Astrophysical Journal 959 (2), 102, 2023 | 1 | 2023 |
| Photometric Classification of Evolved Massive Stars: High-Resolution Spectroscopic Validation I Ghosh-Coutinho, T Dorn-Wallenstein, E Levesque, J Davenport American Astronomical Society Meeting Abstracts 55 (2), 401.31, 2023 | 1 | 2023 |
| arcesetc: ARC Echelle Spectrograph Exposure Time Calculator BM Morris, T Dorn-Wallenstein, EM Levesque, C Sakari, D Gies, K Lester, ... Journal of Open Source Software 4 (34), 1130, 2019 | 1 | 2019 |
| A Spectroscopic Hunt for Post-red Supergiants in the Large Magellanic Cloud. I. Preliminary Results KM Chen, TZ Dorn-Wallenstein Research Notes of the AAS 8 (3), 75, 2024 | | 2024 |
| A Census of Variability in Hot Massive Stars in Gaia and ZTF I Ghosh-Coutinho, J Davenport, T Dorn-Wallenstein, E Levesque American Astronomical Society Meeting Abstracts 56 (2), 205.20, 2024 | | 2024 |
| A Machine Learning Approach to Derive Temperatures and Luminosities for 5000 Cool Supergiants in the LMC from Gaia BP/RP Spectra T Dorn-Wallenstein, K Neugent, E Levesque American Astronomical Society Meeting Abstracts 56 (2), 157.07, 2024 | | 2024 |
| A Spectroscopic Hunt for Post-Red Supergiants in the Large Magellanic Cloud K Chen, T Dorn-Wallenstein American Astronomical Society Meeting Abstracts 56 (2), 205.01, 2024 | | 2024 |
