TOI-2411 Archives

The planetary architectures of the systems WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 are shown from top to bottom. The sizes of the elements in this figure scale with the sizes of the represented stars and planets. The sizes of the stars are scaled relative to each other, and the planets are scaled relative to each other, but the relative scales between stars and planets are not accurate, with planets oversized for clearer visualization. Known planets in the systems are displayed in solid colors, while the candidates found in this study are highlighted with a gray halo and transparency, whose properties are listed in Table 3. -- astro-ph.EP

Astronomy & Telescopes, Exoplanets, -moons, -comets, Imaging & Spectroscopy, Status Report

The SHERLOCK Pipeline: New Exoplanet Candidates In The WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 Systems

by Keith CowingJuly 25, 2024July 25, 2024

The launches of NASA Kepler and TESS missions have significantly enhanced the interest in the exoplanet field during the last 15 years, providing a vast amount of public data that […]

TOI-2411

The SHERLOCK Pipeline: New Exoplanet Candidates In The WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 Systems

Roman Space Telescope: Enabling Images Of Distant Worlds

NASA Solar System Exploration Research Virtual Institute (SSERVI) Cooperative Agreement Notice (NNH26ZDA016C) Final Text And Due Dates

Interstellar Aromatic Infrared Bands: IR Absorption Spectroscopy Of The Lowest Triplet State Of Naphthalene

The Highly Unusual Behavior And Chemical Composition Of Interstellar Comet 2I/Borisov

Volatile Depletion In Rocky Planets As A Chemical Fingerprint Of Hybrid Accretion