195 citations · 542 across the 11 of their papers we have counts for
11 papers
Differential Modelling Systematics across the HR Diagram from Asteroseismic Surface Corrections
J. M. Joel Ong, Sarbani Basu, Jean M. McKeever
Localised modelling error in the near-surface layers of evolutionary stellar models causes the frequencies of their normal modes of oscillation to differ from those of actual stars…
Fast and Automated Peak Bagging with DIAMONDS (FAMED)
E. Corsaro, J. M. McKeever, J. S. Kuszlewicz
Stars of low and intermediate mass that exhibit oscillations may show tens of detectable oscillation modes each. Oscillation modes are a powerful to constrain the internal structur…
Active red giants: close binaries versus single rapid rotators
Patrick Gaulme, Jason Jackiewicz, Federico Spada +7
The objective of this work is to determine what fraction of red-giant (RG) stars shows photometric rotational modulation, and understand its origin. One of the underlying questions…
The Helium Abundance of NGC 6791 from Modeling of Stellar Oscillations
Jean McKeever, Sarbani Basu, Enrico Corsaro
The helium abundance of stars is a strong driver of evolutionary timescales, however it is difficult to measure in cool stars. We conduct an asteroseismic analysis of NGC 6791, an…
Modeling Radial Velocities and Eclipse Photometry of the Kepler Target KIC 4054905: an Oscillating Red Giant in an Eclipsing Binary
M. Benbakoura, P. Gaulme, J. McKeever +3
Asteroseismology is a powerful tool to measure the fundamental properties of stars and probe their interiors. This is particularly efficient for red giants because their modes are…
Testing the asteroseismic scaling relations for Red Giants with Eclipsing Binaries Observed by Kepler
Patrick Gaulme, Jean McKeever, Jason Jackiewicz +7
Given the potential of ensemble asteroseismology for understanding fundamental properties of large numbers of stars, it is critical to determine the accuracy of the scaling relatio…