Ground-based Light Curve Follow-up Validation Observations of TESS Object of Interest TOI 3841.01

Space is a vast and largely unexplored frontier, with the search for exoplanets providing valuable insights into planetary systems beyond our own. NASA’s Transiting Exoplanet Survey Satellite (TESS) mission uses the transit method to analyze stellar light curves in order to identify potential exoplanets. This study focuses on TESS Object of Interest TOI 3841.01, with the goal of generating a light curve and investigating possible transits. Using observational data provided by George Mason University and AstroImageJ, we were able to plate solve and generate a light curve for TOI 3841.01. However, the results were inconclusive due to errors encountered during the data reduction process. Further work, including refined data calibration and analysis, is required to confirm or refute potential transits for this target.