TOI-757 Archives

Mean−subtracted RV data plotted in gray dotted points for each of the HARPS (top panel), ESPRESSO (middle panel), and PFS (bottom panel) instruments, along with separate model curves for the planet model (blue solid line), the GP model (green solid line) and the full planet + GP model (magenta solid line). The error bars include the jitter component 𝜎 for each instrument, which was added in quadrature to the RV error for each data point. -- astro-ph.EP

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

TOI-757 b: An Eccentric Transiting Mini-Neptune On Aa 17.5-d Orbit

by Keith CowingAugust 12, 2024August 10, 2024

We report the spectroscopic confirmation and fundamental properties of TOI-757 b, a mini-Neptune on a 17.5-day orbit transiting a bright star (V=9.7 mag) discovered by the TESS mission. We acquired […]

TOI-757

TOI-757 b: An Eccentric Transiting Mini-Neptune On Aa 17.5-d Orbit

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