Joseph M. Akana Murphy

TL;DR: In this article, the authors reported the detection of a Saturn-size exoplanet orbiting HD 332231 (TOI 1456) in light curves from the Transiting Exoplanet Survey Satellite (TESS).

TL;DR: The discovery of TOI-561, a multi-planar system in the galactic thick disk that contains a rocky, ultra-short-period planet was reported in this article.

TL;DR: In this paper, the authors measured the Rossiter-McLaughlin effect of WASP-107b during a single transit with Keck/HIRES and found the sky-projected inclination relative to its host star's rotation axis, to be $|\lambda| = {118}^{+38}_{-19}$ degrees.

TL;DR: In this article, the authors reported the measurement of a spectroscopic transit of TOI-1726c, one of two planets transiting a G-type star with V = 6.9 in the Ursa Major Moving Group (~400 Myr).

TL;DR: To confirm the TESS planet discovery using reconnaissance spectroscopy, ground-based photometry, high-resolution imaging, and a set of 38 precise radial velocities (RVs) from HARPS-N and HIRES, this article measured a planet mass of 6.91 ± 0.5% at 90% confidence, which implies an iron core mass fraction of 20% in the absence of a gaseous envelope.