Ground-Based Light Curve Follow-Up Validation Observations of TOI 3798.01

Through the NASA TESS mission, the confirmation of exoplanets surrounding their host stars has become a crucial part of scientific investigation in understanding the evolution of planetary systems. The goal of this study is to analyze and confirm the existence of TESS Object of Interest (TOI) 3798.01. The potential validation of this candidate is presented within this paper. This process of research was conducted using software including AstroImageJ, Jupyter Notebook, and the Mikulski Archive for Space Telescopes. Due to the nature of the NASA TESS mission focusing on transit detection, that was the sole method of confirmation used. Throughout this research, it was found that there is not a conclusive transit detection found for TOI-3798.01, however, with increased research and resources, a confirmed conclusion can be determined.