Hot Jupiters were the first exoplanets to be discovered around main sequence stars and
astonished us with their close-in orbits. They are a prime example of how exoplanets have …

Yearslong time series of high-precision brightness measurements have been assembled for
thousands of stars with telescopes operating in space. Such data have allowed astronomers …

We describe the catalogs assembled and the algorithms used to populate the revised TESS
Input Catalog (TIC), based on the incorporation of the Gaia second data release. We also …

The growing field of large-scale time domain astronomy requires methods for probabilistic
data analysis that are computationally tractable, even with large data sets. Gaussian …

Abstract The Transiting Exoplanet Survey Satellite (TESS) will be conducting a nearly all-sky
photometric survey over two years, with a core mission goal to discover small transiting …

Abstract The Transiting Exoplanet Survey Satellite (TESS) has a goal of detecting small
planets orbiting stars bright enough for mass determination via ground-based radial velocity …

We present a methodology for the determination of empirical masses of single stars through
the combination of three direct observables with Gaia and Transiting Exoplanet Survey …

ABSTRACT CHEOPS (CHaracterising ExOPlanet Satellite) is an ESA S-class mission that
observes bright stars at high cadence from low-Earth orbit. The main aim of the mission is to …

We present the first near all-sky yield of oscillating red giants from the prime mission data of
NASA's Transiting Exoplanet Survey Satellite (TESS). We apply machine learning toward …

SDSS-V, the fifth phase of the Sloan Digital Sky Survey (Kollmeier et al., 2017), will be
astronomy's first all-sky, multi-epoch spectroscopic survey, observing the Universe in both …