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In this work, we present the analysis of 33,054 M-dwarf stars located within100 parsecs in the Transiting Exoplanet Survey Satellite (TESS) Full FrameImages (FFIs) of the observed sectors 1 to 5. We present a new pipeline calledNEMESIS which was developed to extract detrended photometry and perform transitsearches of single sector data in TESS FFIs. As many M-dwarfs are faint and arenot observed with a 2 minute cadence by TESS, FFI transit surveys can give anempirical validation of how many planets are missed by using the 30 minutecadence data. In this work, we detected 183 threshold crossing events andpresent 29 planet candidates for sectors 1 to 5, 24 of which are newdetections. Our sample contains orbital periods ranging from 1.25 to 6.84 daysand planetary radii from 1.26 to 5.31 Earth radii. With the addition of our newplanet candidate detections along with previous detections observed in sectors1 to 5, we calculate an integrated occurrence rate of 2.49 +/- 1.58 planets perstar for the period range between [1,9] days and planet radius range between[0.5,11] Earth radii. We project an estimated yield of 122 +/- 11 transitdetections of nearby M-dwarfs. 23 of our new candidates have Signal to Noiseratios > 7, Transmission Spectroscopy Metrics > 38 and Emission SpectroscopyMetrics > 10. We provide all of our data products for our planet candidatesthrough the Filtergraph data visualization service located athttps://filtergraph.com/NEMESIS.

NEMESIS: Exoplanet Transit Survey of Nearby M-Dwarfs in TESS FFIs I