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20192023
most citedOccurrence rate of hot Jupiters around early-type M dwarfs based on TESS data

89 citations · 383 across the 12 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.EP2022★ 72 cited

TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain

Fei Dai, Kento Masuda, Corey Beard +60

Convergent disk migration has long been suspected to be responsible for forming planetary systems with a chain of mean-motion resonances (MMR). Dynamical evolution over time could…

astro-ph.EP2022★ 89 cited

Occurrence rate of hot Jupiters around early-type M dwarfs based on TESS data

Tianjun Gan, Sharon X. Wang, Songhu Wang +26

We present an estimate of the occurrence rate of hot Jupiters (, days) around early-type M dwarfs based on stars obser…

astro-ph.EP2022★ 25 cited

The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets

Samuel W. Yee, Joshua N. Winn, Joel D. Hartman +69

We report the discovery of ten short-period giant planets (TOI-2193A b, TOI-2207 b, TOI-2236 b, TOI-2421 b, TOI-2567 b, TOI-2570 b, TOI-3331 b, TOI-3540A b, TOI-3693 b, TOI-4137 b)…

astro-ph.EP2022★ 34 cited

Validation of 13 Hot and Potentially Terrestrial TESS Planets

Steven Giacalone, Courtney D. Dressing, Christina Hedges +108

The James Webb Space Telescope (JWST) will be able to probe the atmospheres and surface properties of hot, terrestrial planets via emission spectroscopy. We identify 18 potentially…

astro-ph.EP2022★ 27 cited

A transiting, temperate mini-Neptune orbiting the M dwarf TOI-1759 unveiled by TESS

Néstor Espinoza, Enric Pallé, Jonas Kemmer +66

We report the discovery and characterization of TOI-1759~b, a temperate (400 K) sub-Neptune-sized exoplanet orbiting the M~dwarf TOI-1759 (TIC 408636441). TOI-1759 b was observed b…

astro-ph.EP2022★ 41 cited

A Possible Alignment Between the Orbits of Planetary Systems and their Visual Binary Companions

Sam Christian, Andrew Vanderburg, Juliette Becker +111

Astronomers do not have a complete picture of the effects of wide-binary companions (semimajor axes greater than 100 AU) on the formation and evolution of exoplanets. We investigat…