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The NASA High-Resolution Speckle Interferometric Imaging Program: Validation and Characterization of Exoplanets and Their Stellar Hosts
Published 2021-03-01“…Our community program obtains high-resolution imagery, reduces the data, and provides all final data products, without any exclusive use period, to the community via the Exoplanet Follow-Up Observation Program (ExoFOP) website maintained by the NASA Exoplanet Science Institute. This paper describes the need for high-resolution imaging and gives details of the speckle imaging program, highlighting some of the major scientific discoveries made along the way.…”
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Follow-Up and Validation of K2 and TESS Planetary Systems With Keck NIRC2 Adaptive Optics Imaging
Published 2021-06-01Get full text
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Star-crossed Lovers DI Tau A and B: Orbit Characterization and Physical Properties Determination
Published 2023-01-01Get full text
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Scaling K2. VI. Reduced Small-planet Occurrence in High-galactic-amplitude Stars
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Relative Occurrence Rate between Hot and Cold Jupiters as an Indicator to Probe Planet Migration
Published 2024-01-01Get full text
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High-contrast Imaging around a 2 Myr-old CI Tau with a Close-in Gas Giant
Published 2022-01-01Get full text
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A GROUND-BASED OPTICAL TRANSMISSION SPECTRUM OF WASP-6b
Published 2015Get full text
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A THIRD HOT WHITE DWARF COMPANION DETECTED BY KEPLER
Published 2015Get full text
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The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets
Published 2023-01-01Get full text
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The POKEMON Speckle Survey of Nearby M Dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs within 15 pc
Published 2024-01-01Get full text
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The First Evidence of a Host Star Metallicity Cutoff in the Formation of Super-Earth Planets
Published 2024-01-01Get full text
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Scaling K2. VII. Evidence For a High Occurrence Rate of Hot Sub-Neptunes at Intermediate Ages
Published 2023-01-01Get full text
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