Asteroseismology has grown from its beginnings three decades ago to a mature field
teeming with discoveries and applications. This phenomenal growth has been enabled by …

Binary stars are crucial laboratories for stellar physics, so have been photometric targets for
space missions beginning with the very first orbiting telescope (OAO-2) launched in 1968 …

In this paper we present a catalog of 4584 eclipsing binaries observed during the first two
years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binary …

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 …

Post-common envelope binaries (PCEBs) containing a white dwarf (WD) and a main-
sequence (MS) star can constrain the physics of common envelope evolution and calibrate …

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 …

The orbital parameters of binaries at intermediate periods (102–103 d) are difficult to
measure with conventional methods and are very incomplete. We have undertaken a new …

The high-quality light curves from the Transiting Exoplanet Survey Satellite (TESS) represent
a unique laboratory for the study of stellar rotation, which is a fundamental observable …

Context. Stellar evolution models of B-type stars are still uncertain in terms of internal mixing
properties, notably in the area between the convective core and the radiative envelope. This …

The field of visible-light continuous time series photometry is now at its golden age,
manifested by the continuum of past (CoRoT, Kepler), present (K2), and future (TESS …