Context. The Kepler spacecraft is providing time series of photometric data with
micromagnitude precision for hundreds of AF type stars. Aims. We present a first general …

The NASA Kepler and follow-on K2 mission (2009–2018) left a legacy of data and
discoveries, finding thousands of exoplanets, and also obtaining high-precision long time …

We present a new oscillation code, gyre, which solves the stellar pulsation equations (both
adiabatic and non-adiabatic) using a novel Magnus Multiple Shooting numerical scheme …

ABSTRACT The Kepler Mission, launched on 2009 March 6, was designed with the explicit
capability to detect Earth-size planets in the habitable zone of solar-like stars using the …

We study the fraction of stars in and around the δ Scuti instability strip that are pulsating,
using Gaia DR2 parallaxes to derive precise luminosities. We classify a sample of over 15 …

We present the first asteroseismic results for δ Scuti and γ Doradus stars observed in
Sectors 1 and 2 of the TESS mission. We utilize the 2-min cadence TESS data for a sample …

The Kepler mission is providing photometric data of exquisite quality for the asteroseismic
study of different classes of pulsating stars. These analyses place particular demands on the …

The δ Sct stars are a diverse group of intermediate-mass pulsating stars located on and near
the main sequence within the classical instability strip in the Hertzsprung–Russell diagram …

We have found a rotationally split series of core g-mode triplets and surface p-mode
multiplets in a main-sequence F star, KIC 9244992. Comparison with models shows that the …

We present the results of a search for amplitude modulation of pulsation modes in 983 δ Sct
stars, which have effective temperatures between 6400≤ T eff≤ 10 000 K in the Kepler …