activity
20092026
most citedMasses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets

497 citations · 10.4k across the 148 of their papers we have counts for

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Showing 2015Show all

8 papers · 1 filter

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.SR2015★ 154 cited

Oscillation frequencies for 35 \Kepler solar-type planet-hosting stars using Bayesian techniques and machine learning

G. R. Davies, V. Silva Aguirre, T. R. Bedding +16

\Kepler has revolutionised our understanding of both exoplanets and their host stars. Asteroseismology is a valuable tool in the characterisation of stars and \Kepler is an excelle…

astro-ph.SR2015★ 15 cited

Spot cycle reconstruction: an empirical tool - Application to the sunspot cycle

A. R. G. Santos, M. S. Cunha, P. P. Avelino +1

The increasing interest in understanding stellar magnetic activity cycles is a strong motivation for the development of parameterized starspot models which can be constrained obser…

astro-ph.SR2015★ 37 cited

Asteroseismology of solar-type stars with K2

W. J. Chaplin, M. N. Lund, R. Handberg +44

We present the first detections by the NASA K2 Mission of oscillations in solar-type stars, using short-cadence data collected during K2 Campaign\,1 (C1). We understand the asteros…

astro-ph.SR2015★ 407 cited

Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology

V. Silva Aguirre, G. R. Davies, S. Basu +21

We present a study of 33 {\it Kepler} planet-candidate host stars for which asteroseismic observations have sufficiently high signal-to-noise ratio to allow extraction of individua…

astro-ph.SR2015

Asteroseismology of Exoplanet-Host Stars in the Kepler Era

Tiago L. Campante

New insights on stellar evolution and stellar interior physics are being made possible by asteroseismology, the study of stars by the observation of their natural, resonant oscilla…