BANYAN Σ is a new Bayesian algorithm to identify members of young stellar associations
within 150 pc of the Sun. It includes 27 young associations with ages in the range∼ 1–800 …

Over the duration of the Kepler mission, KIC 8462852 was observed to undergo irregularly
shaped, aperiodic dips in flux of up to∼ 20 per cent. The dipping activity can last for …

We outline the impact of a small two-band UV-photometry satellite mission on the field of
stellar physics, magnetospheres of stars, binaries, stellar clusters, interstellar matter, and …

We confirm and characterize a close-in (${P} _ {{\rm {orb}}} $= 5.425 days), super-Neptune
sized (${5.04} _ {-0.37}^{+ 0.34} $${R} _ {\oplus} $) planet transiting K2-33 (2MASS …

We present an analysis of K2 light curves (LCs) for candidate members of the young Upper
Sco (USco) association (∼ 8 Myr) and the neighboring ρ Oph embedded cluster (∼ 1 Myr) …

AA Tau is the archetype for a class of stars with a peculiar periodic photometric variability
thought to be related to a warped inner disk structure with a nearly edge-on viewing …

Abstract The Upper Scorpius OB association is the nearest region of recent massive star
formation and thus an important benchmark for investigations concerning stellar evolution …

We have refined the census of stars and brown dwarfs in the Upper Sco association (∼ 10
Myr,∼ 145 pc) by (1) updating the selection of candidate members from our previous survey …

Sub-Neptunes around FGKM dwarfs are evenly distributed in log orbital period down to∼ 10
days, but dwindle in number at shorter periods. Both the break at∼ 10 days and the slope of …

ABSTRACT HD 139614 is known to be a∼ 14-Myr-old, possibly pre-main-sequence star in
the Sco-Cen OB association in the Upper Centaurus-Lupus subgroup, with a slightly warped …