This work studied 12,993 light curves from stars observed by the Transiting Exoplanet Survey Satellite in autumn 2024 to search for transit signals of exoplanets, tiny dips in brightness, when an exoplanet passes in front of a star and blocks a little of its light. Using visual analysis methods, 139 transit signals were detected. Among them, 10 are known confirmed exoplanets, 121 are candidates, which are potentially exoplanets but not yet confirmed, and 2 are new high-priority exoplanet candidates. These 2 last objects passed validation false-positive tests and may represent new discoveries worth further study. Physical parameters of 133 exoplanets, exoplanet candidates, and host stars were calculated. Most of the exoplanets are gas giants with short orbits around G-class stars.