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19952026
most citedGravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars

612 citations · 8.5k across the 93 of their papers we have counts for

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14 papers · 1 filter

astro-ph.EP2020★ 51 cited

TOI-257b (HD 19916b): A Warm sub-Saturn Orbiting an Evolved F-type Star

Brett C. Addison, Duncan J. Wright, Belinda A. Nicholson +91

We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal was detected by TESS…

astro-ph.EP2019★ 95 cited

A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS

Daniel Huber, William J. Chaplin, Ashley Chontos +139

We present the discovery of TOI-197.01, the first transiting planet identified by the Transiting Exoplanet Survey Satellite (TESS) for which asteroseismology of the host star is po…

astro-ph.EP2016★ 264 cited

Hot super-Earths stripped by their host stars

M. S. Lundkvist, H. Kjeldsen, S. Albrecht +26

Simulations predict that hot super-Earth sized exoplanets can have their envelopes stripped by photo-evaporation, which would present itself as a lack of these exoplanets. However,…

astro-ph.EP2015★ 42 cited

The Kepler-454 System: A Small, Not-rocky Inner Planet, a Jovian World, and a Distant Companion

Sara Gettel, David Charbonneau, Courtney D. Dressing +47

Kepler-454 (KOI-273) is a relatively bright (V = 11.69 mag), Sun-like starthat hosts a transiting planet candidate in a 10.6 d orbit. From spectroscopy, we estimate the stellar tem…

astro-ph.EP2015★ 1 cited

KOI-3158: The oldest known system of terrestrial-size planets

T. L. Campante, T. Barclay, J. J. Swift +38

The first discoveries of exoplanets around Sun-like stars have fueled efforts to find ever smaller worlds evocative of Earth and other terrestrial planets in the Solar System. Whil…

astro-ph.EP2015★ 214 cited

An ancient extrasolar system with five sub-Earth-size planets

T. L. Campante, T. Barclay, J. J. Swift +38

The chemical composition of stars hosting small exoplanets (with radii less than four Earth radii) appears to be more diverse than that of gas-giant hosts, which tend to be metal-r…