2022RNAAS...6..184D

We report an analysis of the TESS light curve of the nearby M dwarf Gl 514 that was observed during Sector 50. We search for a transit of the likely super-Earth Gl 514 b that was detected in 2022 in radial velocity data. The planet moves on an eccentric orbit that partly resides within the habitable zone of its host. According to the predictions, a transit may occur with high probability within the observing window covered by Sector 50, and being easily detected, therefore offering a great opportunity for an independent confirmation of the existence of Gl 514 b, and for a better characterization of the planet.