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20032024
most citedPlanetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months)

264 citations · 2.3k across the 42 of their papers we have counts for

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astro-ph.EP202410 cited

Seasonal Changes in the Atmosphere of HD 80606b Observed with JWST's NIRSpec/G395H

James T. Sikora, Jason F. Rowe, Jared Splinter +11

High-eccentricity gas giant planets serve as unique laboratories for studying the thermal and chemical properties of H/He-dominated atmospheres. One of the most extreme cases is HD…

astro-ph.EP20241 cited

JWST Directly Images Giant Planet Candidates Around Two Metal-Polluted White Dwarf Stars

Susan E. Mullally, John Debes, Misty Cracraft +9

We report the discovery of two directly imaged, giant planet candidates orbiting the metal-rich DAZ white dwarfs WD 1202-232 and WD 2105-82. JWST's Mid-Infrared Instrument (MIRI) d…

astro-ph.EP2023

A MIRI Search for Planets and Dust Around WD 2149+02

Sabrina Poulsen, John Debes, Misty Cracraft +9

The launch of JWST has ushered in a new era of high precision infrared astronomy, allowing us to probe nearby white dwarfs for cold dust, exoplanets, and tidally heated exomoons. W…

astro-ph.EP2023

Transiting Exoplanet Yields for the Roman Galactic Bulge Time Domain Survey Predicted from Pixel-Level Simulations

Robert F. Wilson, Thomas Barclay, Brian P. Powell +8

The Nancy Grace Roman Space Telescope (Roman) is NASA's next astrophysics flagship mission, expected to launch in late 2026. As one of Roman's core community science surveys, the G…

astro-ph.EP2023

Two Warm Super-Earths Transiting the Nearby M Dwarf TOI-2095

Elisa V. Quintana, Emily A. Gilbert, Thomas Barclay +55

We report the detection and validation of two planets orbiting TOI-2095 (TIC 235678745). The host star is a 3700K M1V dwarf with a high proper motion. The star lies at a distance o…

astro-ph.EP202225 cited

A transmission spectrum of the sub-Earth planet L98-59~b in 1.1-1.7 m

Mario Damiano, Renyu Hu, Thomas Barclay +20

With the increasing number of planets discovered by TESS, the atmospheric characterization of small exoplanets is accelerating. L98-59 is a M-dwarf hosting a multi-planet system, a…