Search Results for author: Timothy R. Bedding

Found 4 papers, 3 papers with code

The K2 Bright Star Survey I: Methodology and Data Release

1 code implementation19 Aug 2019 Benjamin J. S. Pope, Timothy R. White, Will M. Farr, Jie Yu, Michael Greklek-McKeon, Daniel Huber, Conny Aerts, Suzanne Aigrain, Timothy R. Bedding, Tabetha Boyajian, Orlagh L. Creevey, David W. Hogg

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 been observed very accurately by other instruments.

Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics

Asteroseismology of the Hyades red giant and planet host epsilon Tauri

no code implementations18 Jan 2019 Torben Arentoft, Frank Grundahl, Timothy R. White, Ditte Slumstrup, Rasmus Handberg, Mikkel N. Lund, Karsten Brogaard, Mads F. Andersen, Victor Silva Aguirre, Chunguang Zhang, Xiaodian Chen, Zhengzhou Yan, Benjamin J. S. Pope, Daniel Huber, Hans Kjeldsen, Jørgen Christensen-Dalsgaard, Jens Jessen-Hansen, Victoria Antoci, Søren Frandsen, Timothy R. Bedding, Pere L. Palle, Rafael A. Garcia, Licai Deng, Marc Hon, Dennis Stello, Uffe G. Jørgensen

Using asteroseismic techniques combined with other methods, we aim to derive physical parameters and the evolutionary stage for the planet hosting star epsilon Tau, which is one of the four red giants located in the Hyades.

Solar and Stellar Astrophysics

Asteroseismology of 16000 Kepler Red Giants: Global Oscillation Parameters, Masses, and Radii

2 code implementations13 Feb 2018 Jie Yu, Daniel Huber, Timothy R. Bedding, Dennis Stello, Marc Hon, Simon J. Murphy, Shourya Khanna

Thanks to the large red giant sample, we confirm that red-giant-branch (RGB) and helium-core-burning (HeB) stars collectively differ in the distribution of oscillation amplitude, granulation power, and width of power excess, which is mainly due to the mass difference.

Solar and Stellar Astrophysics

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