activity
20052026
most citedPlanetary Candidates Observed by Kepler, III: Analysis of the First 16 Months of Data

1.1k citations · 15.4k across the 165 of their papers we have counts for

collaborators
Showing 2019 · astro-ph.EPShow all

9 papers · 2 filters

astro-ph.EP2019★ 18 cited

TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS

Allen B. Davis, Songhu Wang, Matias Jones +46

We report the discovery and confirmation of two new hot Jupiters discovered by the Transiting Exoplanet Survey Satellite (TESS): TOI 564 b and TOI 905 b. The transits of these two…

astro-ph.EP2019★ 121 cited

Two new HATNet hot Jupiters around A stars, and the first glimpse at the occurrence rate of hot Jupiters from TESS

G. Zhou, C. X. Huang, G. Á. Bakos +68

Wide field surveys for transiting planets are well suited to searching diverse stellar populations, enabling a better understanding of the link between the properties of planets an…

astro-ph.EP2019★ 98 cited

Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M Dwarf System at 6.9 Parsecs

Jennifer G. Winters, Amber A. Medina, Jonathan M. Irwin +40

We present the discovery from TESS data of LTT 1445Ab. At a distance of 6.9 parsecs, it is the second nearest transiting exoplanet system found to date, and the closest one known f…

astro-ph.EP2019★ 4 cited

A Hot Saturn Near (but unassociated with) the Open Cluster NGC 1817

Rayna Rampalli, Andrew Vanderburg, Allyson Bieryla +14

We report on the discovery of a hot Saturn-sized planet (9.916 +/- 0.985 R_earth) around a late F star, EPIC 246865365, observed in Campaign 13 of the K2 mission. We began studying…

astro-ph.EP2019★ 23 cited

KELT-24b: A 5M Planet on a 5.6 day Well-Aligned Orbit around the Young V=8.3 F-star HD 93148

Joseph E. Rodriguez, Jason D. Eastman, George Zhou +76

We present the discovery of KELT-24 b, a massive hot Jupiter orbiting a bright (V=8.3 mag, K=7.2 mag) young F-star with a period of 5.6 days. The host star, KELT-24 (HD 93148), has…

astro-ph.EP2019★ 36 cited

TOI-216b and TOI-216c: Two warm, large exoplanets in or slightly wide of the 2:1 orbital resonance

Rebekah I. Dawson, Chelsea X. Huang, Jack J. Lissauer +32

Warm, large exoplanets with 10-100 day orbital periods pose a major challenge to our understanding of how planetary systems form and evolve. Although high eccentricity tidal migrat…