TOI-6324 b Archives

Ground-based light curves from LCOGT, KeplerCam, and MUSCAT2. The colored data points correspond to the binned data at 5 minute cadence. The solid black line is the median model from the posterior distribution. The solid blue curve is the median TESS light curve projected into the corresponding band. -- astro-ph.EP

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

Validation of TESS Planet Candidates with Multi-Color Transit Photometry and TRICERATOPS+

by Keith CowingAugust 8, 2025August 8, 2025

We present an upgraded version of TRICERATOPS, a software package designed to calculate false positive probabilities for planet candidates identified by the Transiting Exoplanet Survey Satellite (TESS).

Binned and phase-folded SPOC PDC-SAP light curve of TOI-6324 revealing the transit signal of TOI-6324 b, with the best-fit transit model over-plotted in blue. The residuals (data minus model) are shown in the bottom panel. -- astro-ph.EP

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

TOI-6324b: An Earth-Mass Ultra-Short-Period Planet Transiting a Nearby M Dwarf

by Keith CowingMarch 4, 2025March 4, 2025

We report the confirmation of TOI-6324 b, an Earth-sized (1.059 ± 0.041 R⊕) ultra-short-period (USP) planet orbiting a nearby (∼20 pc) M dwarf.

TOI-6324 b

Validation of TESS Planet Candidates with Multi-Color Transit Photometry and TRICERATOPS+

TOI-6324b: An Earth-Mass Ultra-Short-Period Planet Transiting a Nearby M Dwarf

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