activity
20152021
most citedWeakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs

94 citations · 556 across the 12 of their papers we have counts for

collaborators

17 papers

astro-ph.SR202124 cited

Hierarchically modelling Kepler dwarfs and subgiants to improve inference of stellar properties with asteroseismology

Alexander J. Lyttle, Guy R. Davies, Tanda Li +9

With recent advances in modelling stars using high-precision asteroseismology, the systematic effects associated with our assumptions of stellar helium abundance () and the mixi…

astro-ph.SR202194 cited

Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs

Oliver J. Hall, Guy R. Davies, Jennifer van Saders +9

Studies using asteroseismic ages and rotation rates from star-spot rotation have indicated that standard age-rotation relations may break down roughly half-way through the main seq…

astro-ph.SR202132 cited

ROOSTER: a machine-learning analysis tool for Kepler stellar rotation periods

Sylvain N. Breton, Angela R. G. Santos, Lisa Bugnet +3

In order to understand stellar evolution, it is crucial to efficiently determine stellar surface rotation periods. An efficient tool to automatically determine reliable rotation pe…

astro-ph.SR202028 cited

The K2 Galactic Archaeology Program Data Release 2: Asteroseismic results from campaigns 4, 6, & 7

Joel C. Zinn, Dennis Stello, Yvonne Elsworth +18

Studies of Galactic structure and evolution have benefitted enormously from Gaia kinematic information, though additional, intrinsic stellar parameters like age are required to bes…

astro-ph.SR2020

Robust asteroseismic properties of the bright planet host HD 38529

Warrick H. Ball, William J. Chaplin, Martin B. Nielsen +21

The Transiting Exoplanet Survey Satellite (TESS) is recording short-cadence, high duty-cycle timeseries across most of the sky, which presents the opportunity to detect and study o…

astro-ph.SR2020

Investigating surface correction relations for RGB stars

Andreas Christ Sølvsten Jørgensen, Josefina Montalbán, Andrea Miglio +7

State-of-the-art stellar structure and evolution codes fail to adequately describe turbulent convection. For stars with convective envelopes, such as red giants, this leads to an i…