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David Charbonneau

David Charbonneau

· Professor

Harvard University · Astronomy

Active 1998–2025

h-index112
Citations52.3k
Papers711181 last 5y
Funding$2.2M

Academic metrics are sourced from OpenAlex and public funding records; values may differ from Google Scholar.

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About

David Charbonneau is the Fred Kavli Professor of Astrophysics and the Chair of the Department of Astronomy at Harvard University. His research interests focus on the detection and characterization of extrasolar planets, with the overarching goal of studying inhabited worlds. In pursuit of this goal, he also engages in the development of novel ground-based and space-based instrumentation, as well as studies of stellar astrophysics. His work aims to advance understanding of planetary systems beyond our own and to contribute to the broader field of astrophysics through innovative observational techniques and instrumentation.

Research topics

  • Astronomy
  • Physics
  • Computer Science
  • Computer Security
  • Artificial Intelligence
  • Astrophysics
  • Astrobiology
  • Mathematics

Selected publications

  • The TESS Objects of Interest Catalog from the TESS Prime Mission

    The Astrophysical Journal Supplement Series · 2021 · 300 citations

    We present 2241 exoplanet candidates identified with data from the Transiting Exoplanet Survey Satellite (TESS) during its 2 yr Prime Mission. We list these candidates in the TESS Objects of Interest (TOI) Catalog, which includes both new planet candidates found by TESS and previously known planets recovered by TESS observations. We describe the process used to identify TOIs, investigate the characteristics of the new planet candidates, and discuss some notable TESS planet discoveries. The TOI c…

  • Vetting of 384 TESS Objects of Interest with TRICERATOPS and Statistical Validation of 12 Planet Candidates

    The Astronomical Journal · 2020 · 153 citations

    Abstract We present TRICERATOPS , a new Bayesian tool that can be used to vet and validate TESS Objects of Interest (TOIs). We test the tool on 68 TOIs that have been previously confirmed as planets or rejected as astrophysical false positives. By looking in the false-positive probability (FPP)−nearby false-positive probability (NFPP) plane, we define criteria that TOIs must meet to be classified as validated planets (FPP < 0.015 and NFPP < 10 −3 ), likely planets (FPP < 0.5 and NFPP &l…

  • A Pair of TESS Planets Spanning the Radius Valley around the Nearby Mid-M Dwarf LTT 3780

    The Astronomical Journal · 2020 · 96 citations

    Abstract We present the confirmation of two new planets transiting the nearby mid-M dwarf LTT 3780 (TIC 36724087, TOI-732, V = 13.07, K s = 8.204, R s = 0.374 R ⊙ , M s = 0.401 M ⊙ , d = 22 pc). The two planet candidates are identified in a single Transiting Exoplanet Survey Satellite sector and validated with reconnaissance spectroscopy, ground-based photometric follow-up, and high-resolution imaging. With measured orbital periods of P b = 0.77, P c = 12.25 days and sizes r p , b = 1.33 ± 0.07,…

  • TOI-836: A super-Earth and mini-Neptune transiting a nearby K-dwarf

    Monthly Notices of the Royal Astronomical Society · 2023 · 27 citations

    ABSTRACT We present the discovery of two exoplanets transiting TOI-836 (TIC 440887364) using data from TESS Sector 11 and Sector 38. TOI-836 is a bright (T = 8.5 mag), high proper motion (∼200 mas yr−1), low metallicity ([Fe/H]≈−0.28) K-dwarf with a mass of 0.68 ± 0.05 M⊙ and a radius of 0.67 ± 0.01 R⊙. We obtain photometric follow-up observations with a variety of facilities, and we use these data sets to determine that the inner planet, TOI-836 b, is a 1.70 ± 0.07 R⊕ super-Earth in a 3.82-d or…

  • The Receding Cosmic Shoreline of Mid-to-late M Dwarfs: Measurements of Active Lifetimes Worsen Challenges for Atmosphere Retention by Rocky Exoplanets

    The Astrophysical Journal Letters · 2025-06-03 · 16 citations

    articleOpen access

    Abstract Detecting and characterizing the atmospheres of terrestrial exoplanets is a key goal of exoplanetary astronomy, one that may now be within reach given the upcoming campaign to conduct a large-scale survey of rocky M-dwarf worlds with the James Webb Space Telescope. It is imperative that we understand where known planets sit relative to the cosmic shoreline—the boundary between planets that have retained atmospheres and those that have not. Previous works modeled the historic X-ray and u…

Recent grants

Frequent coauthors

  • David W. Latham

    269 shared
  • Sara Seager

    Massachusetts Institute of Technology

    234 shared
  • Timothy M. Brown

    Brigham Young University

    164 shared
  • Jonathan Irwin

    163 shared
  • Lars A. Buchhave

    155 shared
  • Jon M. Jenkins

    153 shared
  • S. Udry

    139 shared
  • David R. Ciardi

    NASA Exoplanet Science Institute

    135 shared

Labs

Education

  • Ph.D., Astronomy

    Harvard University

    1996
  • B.A., Physics

    Princeton University

    1991

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