TESS-Gaia Light Curve pipeline Archives

Number of light curves for stars in LOPS2 classified per TESS sector. The entire bin height indicates all light curves for a given sector, where those with a dominant instrumental frequency f1 are indicated in purple and those with a second or third instrumental frequency (without double counting) in teal. The burgundy dotted line delineates classified nominal and extended mission data. -- astro-ph.SR

Astronomy & Telescopes, Exoplanets, -moons, -comets, PLATO, Status Report, Stellar Cartography

Variability Classification Of TESS Targets in LOPS2, The First Long-term Pointing Field Of PLATO. Version 1 of The Public Variability Catalogue

by Keith CowingApril 17, 2026April 27, 2026

The PLAnetary Transits and Oscillations of stars (PLATO) mission is expected to launch in January 2027. A total of 8\% of its data rate will be dedicated to complementary science […]

TESS-Gaia Light Curve pipeline

Variability Classification Of TESS Targets in LOPS2, The First Long-term Pointing Field Of PLATO. Version 1 of The Public Variability Catalogue

The Polana-Eulalia Complex with JWST NIRSpec: Connections to Bennu, Ryugu, and Outer Solar System Bodies

Planet-wide, Concentric Density Waves in Venus’s Upper Atmosphere Revealed through Polarimetry?

Molecule-dependent Abundance Behavior of Oxygen-bearing Complex Organics in High-Mass Star-Forming Regions: A Uniform 50-source Survey

Optimal Mode-sorting Coronagraphy: Limits Of Single-moded Measurements For The Habitable Worlds Observatory

A Dual-Burst Geometrical Prescription For Concurrent Signaling