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Geert Barentsen

Researcher at Ames Research Center

Publications -  143
Citations -  11516

Geert Barentsen is an academic researcher from Ames Research Center. The author has contributed to research in topics: Exoplanet & Planet. The author has an hindex of 30, co-authored 141 publications receiving 8696 citations. Previous affiliations of Geert Barentsen include Max Planck Society & University of Hertfordshire.

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The L 98-59 System: Three Transiting, Terrestrial-size Planets Orbiting a Nearby M Dwarf

Veselin B. Kostov, +121 more
TL;DR: The transiting exoplanet Survey Satellite (TESS) discovery of three terrestrial-size planets transiting L 98-59 (TOI-175, TIC 307210830) is reported in this article.
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Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations

Wenxiong Li, +183 more
TL;DR: The first spectroscopically confirmed type Ia supernova (ASASSN-18bt) was observed in the Kepler field by Dimitriadis et al. as mentioned in this paper.
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Campaign 9 of the K2 Mission: Observational Parameters, Scientific Drivers, and Community Involvement for a Simultaneous Space- and Ground-based Microlensing Survey

Calen B. Henderson, +126 more
TL;DR: The demographic questions that can be addressed by this program, including the frequency of FFPs and the Galactic distribution of exoplanets, the observational parameters of K2C9, and the array of resources dedicated to concurrent observations are detailed.
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Seeing Double: ASASSN-18bt Exhibits a Two-component Rise in the Early-time K2 Light Curve

Benjamin J. Shappee, +136 more
TL;DR: In this paper, the authors present the discovery of ASASSN-18bt, the K2 light curve, and prediscovery data from ASAS-SN and the Asteroid Terrestrial-impact Last Alert System.
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The Occurrence of Rocky Habitable-zone Planets around Solar-like Stars from Kepler Data

Steve Bryson, +93 more
TL;DR: In this article, the authors presented the first analysis in terms of star-dependent instellation flux, which allows us to track HZ planets, and they found that the HZ occurrence of planets with radius between 0.5 and 1.5 R orbiting stars with effective temperatures between 4800 K and 6300 K. They also presented occurrence rates for various stellar populations and planet size ranges.