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20132023
most citedK2SC: Flexible systematics correction and detrending of K2 light curves using Gaussian Process regression

194 citations · 1.3k across the 32 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

astro-ph.SR2019★ 53 cited

Low-frequency variability in massive stars: Core generation or surface phenomenon?

Daniel Lecoanet, Matteo Cantiello, Eliot Quataert +6

Bowman et al. (2019) reported low-frequency photometric variability in 164 O- and B-type stars observed with K2 and TESS. They interpret these motions as internal gravity waves, wh…

astro-ph.IM2019★ 21 cited

Extended Aperture Photometry of K2 RR Lyrae stars

Emese Plachy, László Molnár, Attila Bódi +6

The \textit{Kepler} space telescope observed thousands of RR Lyrae stars in the K2 mission. In this paper we present our photometric solutions using extended apertures in order to…

astro-ph.SR2019★ 21 cited

The K2 Bright Star Survey I: Methodology and Data Release

Benjamin J. S. Pope, Timothy R. White, Will M. Farr +9

While the Kepler Mission was designed to look at tens of thousands of faint stars (V > 12), brighter stars that saturated the detector are important because they can be and have be…

astro-ph.SR2019★ 10 cited

The Kepler Smear Campaign: Light curves for 102 Very Bright Stars

Benjamin J. S. Pope, Guy R. Davies, Keith Hawkins +19

We present the first data release of the Kepler Smear Campaign, using collateral 'smear' data obtained in the Kepler four-year mission to reconstruct light curves of 102 stars too…

astro-ph.SR2019★ 165 cited

Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry

Dominic M. Bowman, Siemen Burssens, May G. Pedersen +14

Almost all massive stars explode as supernovae and form a black hole or neutron star. The remnant mass and the impact of the chemical yield on subsequent star formation and galacti…

astro-ph.SR2019★ 26 cited

Asteroseismology of the Hyades red giant and planet host epsilon Tauri

Torben Arentoft, Frank Grundahl, Timothy R. White +23

Asteroseismic analysis of solar-like stars allows us to determine physical parameters such as stellar mass, with a higher precision compared to most other methods. Even in a well-s…