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20032015
most citedSolar-like oscillations in low-luminosity red giants: first results from Kepler

241 citations · 941 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.IM2015

Serendipitous Science from the K2 Mission

Derek L. Buzasi, Lindsey Carboneau, Carly Hessler +2

The K2 mission is a repurposed use of the Kepler spacecraft to perform high-precision photometry of selected fields in the ecliptic. We have developed an aperture photometry pipeli…

astro-ph.SR2010★ 199 cited

Asteroseismology of red giants from the first four months of Kepler data: Global oscillation parameters for 800 stars

D. Huber, T. R. Bedding, D. Stello +19

We have studied solar-like oscillations in ~800 red-giant stars using Kepler long-cadence photometry. The sample includes stars ranging in evolution from the lower part of the red-…

astro-ph.SR2010★ 120 cited

Solar-like oscillations in red giants observed with Kepler: comparison of global oscillation parameters from different methods

S. Hekker, Y. Elsworth, J. De Ridder +20

The large number of stars for which uninterrupted high-precision photometric timeseries data are being collected with \textit{Kepler} and CoRoT initiated the development of automat…

astro-ph.SR2010★ 241 cited

Solar-like oscillations in low-luminosity red giants: first results from Kepler

T. R. Bedding, D. Huber, D. Stello +47

We have measured solar-like oscillations in red giants using time-series photometry from the first 34 days of science operations of the Kepler Mission. The light curves, obtained w…

astro-ph.SR2010★ 154 cited

The asteroseismic potential of Kepler: first results for solar-type stars

W. J. Chaplin, T. Appourchaux, Y. Elsworth +105

We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5d of science operations, reveal hi…

astro-ph2008★ 39 cited

Polaris the Cepheid returns: 4.5 years of monitoring from ground and space

H. Bruntt, N. R. Evans, D. Stello +6

We present the analysis of 4.5 years of nearly continuous observations of the classical Cepheid Polaris, which comprise the most precise data available for this star. We have made…