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20192026
most citedexoplanet: Gradient-based probabilistic inference for exoplanet data & other astronomical time series

215 citations · 1.9k across the 57 of their papers we have counts for

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Showing 2020Show all

8 papers · 1 filter

astro-ph.SR2020★ 41 cited

On the first Sct--roAp hybrid pulsator and the stability of p and g modes in chemically peculiar A/F stars

Simon J. Murphy, Hideyuki Saio, Masahide Takada-Hidai +4

Strong magnetic fields in chemically peculiar A-type (Ap) stars typically suppress low-overtone pressure modes (p modes) but allow high-overtone p modes to be driven. KIC 11296437…

astro-ph.SR2020★ 51 cited

The effect of tides on near-core rotation: analysis of 35 Kepler Doradus stars in eclipsing and spectroscopic binaries

Gang Li, Zhao Guo, Jim Fuller +4

We systematically searched for gravity- and Rossby-mode period spacing patterns in Kepler eclipsing binaries with Doradus pulsators. These stars provide an excellent opportunit…

astro-ph.SR2020★ 15 cited

Asteroseismic masses of four evolved planet-hosting stars using SONG and TESS: resolving the retired A-star mass controversy

Sai Prathyusha Malla, Dennis Stello, Daniel Huber +12

The study of planet occurrence as a function of stellar mass is important for a better understanding of planet formation. Estimating stellar mass, especially in the red giant regim…

astro-ph.SR2020★ 212 cited

Physics of Eclipsing Binaries. V. General Framework for Solving the Inverse Problem

Kyle E Conroy, Angela Kochoska, Daniel Hey +6

PHOEBE 2 is a Python package for modeling the observables of eclipsing star systems, but until now has focused entirely on the forward-model -- that is, generating a synthetic mode…

astro-ph.SR2020★ 114 cited

Very regular high-frequency pulsation modes in young intermediate-mass stars

Timothy R. Bedding, Simon J. Murphy, Daniel R. Hey +33

Asteroseismology is a powerful tool for probing the internal structures of stars by using their natural pulsation frequencies. It relies on identifying sequences of pulsation modes…

astro-ph.SR2020★ 18 cited

Forward modeling the orbits of companions to pulsating stars from their light travel time variations

Daniel R. Hey, Simon J. Murphy, Daniel Foreman-Mackey +3

Mutual gravitation between a pulsating star and an orbital companion leads to a time-dependent variation in path length for starlight traveling to Earth. These variations can be us…