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Scaling relations of convective granulation noise across the HR diagram from 3D stellar atmosphere models
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The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations
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Asteroseismology of 36 Kepler subgiants – I. Oscillation frequencies, linewidths, and amplitudes
Yaguang Li, Timothy R Bedding, Tanda Li, et al. Monthly Notices of the Royal Astronomical Society 495(2) 2363 (2020) https://doi.org/10.1093/mnras/staa1335
A Hot Saturn Orbiting an Oscillating Late Subgiant Discovered by TESS
Daniel Huber, William J. Chaplin, Ashley Chontos, Hans Kjeldsen, Jørgen Christensen-Dalsgaard, Timothy R. Bedding, Warrick Ball, Rafael Brahm, Nestor Espinoza, Thomas Henning, Andrés Jordán, Paula Sarkis, Emil Knudstrup, Simon Albrecht, Frank Grundahl, Mads Fredslund Andersen, Pere L. Pallé, Ian Crossfield, Benjamin Fulton, Andrew W. Howard, Howard T. Isaacson, Lauren M. Weiss, Rasmus Handberg, Mikkel N. Lund, Aldo M. Serenelli, et al. The Astronomical Journal 157(6) 245 (2019) https://doi.org/10.3847/1538-3881/ab1488
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Convective-core Overshoot and Suppression of Oscillations: Constraints from Red Giants in NGC 6811
T. Arentoft, K. Brogaard, J. Jessen-Hansen, V. Silva Aguirre, H. Kjeldsen, J. R. Mosumgaard and E. L. Sandquist The Astrophysical Journal 838(2) 115 (2017) https://doi.org/10.3847/1538-4357/aa63f7
Dipole modes with depressed amplitudes in red giants are mixed modes
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T. L. Campante, M. Schofield, J. S. Kuszlewicz, L. Bouma, W. J. Chaplin, D. Huber, J. Christensen-Dalsgaard, H. Kjeldsen, D. Bossini, T. S. H. North, T. Appourchaux, D. W. Latham, J. Pepper, G. R. Ricker, K. G. Stassun, R. Vanderspek and J. N. Winn The Astrophysical Journal 830(2) 138 (2016) https://doi.org/10.3847/0004-637X/830/2/138
Hydrodynamical model atmospheres: Their impact on stellar spectroscopy and asteroseismology of late‐type stars
Suppression of Quadrupole and Octupole Modes in Red Giants Observed by Kepler
Dennis Stello, Matteo Cantiello, Jim Fuller, Rafael A. Garcia and Daniel Huber Publications of the Astronomical Society of Australia 33 (2016) https://doi.org/10.1017/pasa.2016.9
Magnetic variability in the young solar analog KIC 10644253
Oscillation frequencies for 35Keplersolar-type planet-hosting stars using Bayesian techniques and machine learning
G. R. Davies, V. Silva Aguirre, T. R. Bedding, et al. Monthly Notices of the Royal Astronomical Society 456(2) 2183 (2016) https://doi.org/10.1093/mnras/stv2593
Asteroseismology of 1523 misclassified red giants usingKeplerdata
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Nearly uniform internal rotation of solar-like main-sequence stars revealed by space-based asteroseismology and spectroscopic measurements
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Asteroseismology can reveal strong internal magnetic fields in red giant stars
Determining stellar macroturbulence using asteroseismic rotational velocities from Kepler
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THE ROLE OF TURBULENT PRESSURE AS A COHERENT PULSATIONAL DRIVING MECHANISM: THE CASE OF THE δ SCUTI STAR HD 187547
DETECTION OF ℓ = 4 AND ℓ = 5 MODES IN 12 YEARS OF SOLAR VIRGO-SPM DATA—TESTS ONKEPLEROBSERVATIONS OF 16 Cyg A AND B
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WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS A SMALL NEPTUNE AROUND A BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY
A Bayesian approach to scaling relations for amplitudes of solar-like oscillations in Kepler stars
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