KOI 1271.01 Archives

Best-fit transit models for all 8 of the visible transits within Kepler of KOI 1271.01. Overlaid with the models is a scatter plot of the normalized flux values for the 4-day window with the associated error bars given by Kepler. The models were found using EXOPLANET, and the only parameter that was fit for was the time of center transit. The title of each subplot is the epoch number along with the best-fit time of the transit center. We fit the models over a 4-day range around the predicted time of transit using the ephemeris of KOI 1271.01. Therefore, the location of the transit within the window gives a hint of the order of magnitude of the epoch’s TTV. -- astro-ph.EP

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

Single Transit Detection In Kepler With Machine Learning And Onboard Spacecraft Diagnostics

by Keith CowingMarch 9, 2024September 18, 2025

Exoplanet discovery at long orbital periods requires reliably detecting individual transits without additional information about the system. Techniques like phase-folding of light curves and periodogram analysis of radial velocity data […]

KOI 1271.01

Single Transit Detection In Kepler With Machine Learning And Onboard Spacecraft Diagnostics

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