Abstract In this work, we present an analysis of 33,054 M-dwarf stars, located within 100 parsecs, via the Transiting Exoplanet Survey Satellite (TESS) full-frame images (FFIs) observed sectors 1–5. We a new pipeline called NEMESIS, developed to extract detrended photometry, and perform transit searches single-sector data in TESS FFIs. As many M-dwarfs are faint, not with two-minute cadence by ...
