Jerome A. Orosz

TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1–26

The TESS light curve of AI Phoenicis

KEPLER-1647B: THE LARGEST AND LONGEST-PERIOD KEPLER TRANSITING CIRCUMBINARY PLANET

KEPLER 453 b—THE 10th<i>KEPLER</i>TRANSITING CIRCUMBINARY PLANET

TIME VARIATION OF<i>KEPLER</i>TRANSITS INDUCED BY STELLAR SPOTS—A WAY TO DISTINGUISH BETWEEN PROGRADE AND RETROGRADE MOTION. II. APPLICATION TO KOIs

MASSES, RADII, AND ORBITS OF SMALL <i>KEPLER</i> PLANETS: THE TRANSITION FROM GASEOUS TO ROCKY PLANETS

KEPLER-413B: A SLIGHTLY MISALIGNED, NEPTUNE-SIZE TRANSITING CIRCUMBINARY PLANET

Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone

Transiting circumbinary planets Kepler-34 b and Kepler-35 b

Kepler-47: A Transiting Circumbinary Multiplanet System

<i>KEPLER</i>ECLIPSING BINARY STARS. III. CLASSIFICATION OF<i>KEPLER</i>ECLIPSING BINARY LIGHT CURVES WITH LOCALLY LINEAR EMBEDDING