The rotation of a star and the revolutions of its planets are not necessarily aligned. This
article reviews the measurement techniques, key findings, and theoretical interpretations …

We present a systematic search for transiting giant planets () orbiting nearby low-mass stars
(). The formation of giant planets around low-mass stars is predicted to be rare by the core …

Population studies of exoplanets are key to unlocking their statistical properties. So far, the
inferred properties have been mostly limited to planetary, orbital, and stellar parameters …

Over the past three decades, we have witnessed one of the great revolutions in our
understanding of the cosmos—the dawn of the Exoplanet Era. Where once we knew of just …

Ground-based high-resolution spectroscopy (HRS) has detected numerous chemical
species and atmospheric dynamics in exoplanets, most notably ultrahot Jupiters (UHJs) …

We provide a database of transit times and updated ephemerides for 382 planets based on
data from the NASA Transiting Exoplanet Survey Satellite (TESS) and previously reported …

We present estimates for the occurrence rates of hot Jupiters around dwarf stars based on
data from the Transiting Exoplanet Survey Satellite (TESS) Prime Mission. We take 97 hot …

Close binaries suppress the formation of circumstellar (S-type) planets and therefore
significantly bias the inferred planet occurrence rates and statistical trends. After compiling …

The carbon-to-oxygen (C/O) ratio in an exoplanet atmosphere has been suggested as a
potential diagnostic of planet formation. Now that a number of exoplanets have measured …

While cooler giant planets are often observed with nonzero eccentricities, the short-period
circular orbits of hot Jupiters suggest that they lose orbital energy and angular momentum …