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20112026
most citedMasses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets

497 citations · 2k across the 89 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.EP2019★ 72 cited

Radial velocity confirmation of K2-100b: a young, highly irradiated, and low density transiting hot Neptune

O. Barragán, S. Aigrain, D. Kubyshkina +37

We present a detailed analysis of HARPS-N radial velocity observations of K2-100, a young and active star in the Praesepe cluster, which hosts a transiting planet with a period of…

astro-ph.SR2019★ 28 cited

The compact multiple system HIP 41431

T. Borkovits, J. Sperauskas, A. Tokovinin +4

The nearby (50 pc) K7V dwarf HIP~41431 (EPIC 212096658) is a compact 3-tier hierarchy. Three K7V stars with similar masses, from 0.61 to 0.63 solar, make a triple-lined spectroscop…

astro-ph.SR2019★ 53 cited

Complex Rotational Modulation of Rapidly Rotating M-Stars Observed with TESS

Z. Zhan, M. N. Günther, S. Rappaport +23

We have searched for short periodicities in the light curves of stars with cooler than 4000 K made from 2-minute cadence data obtained in TESS sectors 1 and 2. Herein…

astro-ph.EP2019★ 12 cited

KELT-23Ab: A Hot Jupiter Transiting a Near-Solar Twin Close to the TESS and JWST Continuous Viewing Zones

Daniel Johns, Phillip Reed, Joseph Rodriguez +55

We announce the discovery of KELT-23Ab, a hot Jupiter transiting the relatively bright () star BD+66 911 (TYC 4187-996-1), and characterize the system using follow-up photo…

astro-ph.SR2019★ 29 cited

Deep Long Asymmetric Occultation in EPIC 204376071

S. Rappaport, G. Zhou, A. Vanderburg +15

We have discovered a young M star of mass and radius , likely in the Upper Sco Association, that exhibits only a single deep occultation of 1-…

astro-ph.EP2019★ 17 cited

So close, so different: characterization of the K2-36 planetary system with HARPS-N

M. Damasso, L. Zeng, L. Malavolta +19

K2-36 is a K dwarf orbited by two small ( and ), close-in (=0.022 AU and =0.054 AU) transiti…