Plavchan, PeterCollins, KevinXiao, Cindy2024-04-172024-04-172023-10http://hdl.handle.net/1920/13602https://doi.org/10.13021/MARS/2062Context The best-fit light curve model helps determine various characteristics of the exoplanet, such as its orbital period, radius, and sometimes even its atmospheric properties. Aims Conducting an analysis and interpretation of light curves derived from the provided dataset. The dataset contains various parameters for each observed slice of data, including saturated labels, Julian Dates, Heliocentric Julian Dates, Barycentric Julian Dates, air mass, object altitude, CCD temperature, exposure time, object coordinates, full width at half maximum (FWHM), source and sky radii, relative flux measurements, and associated errors for multiple comparison stars (C1 to C11) and the target star (T1). Methods Methodology employed for data processing, the extraction of photometric information, and the calculation of relevant parameters for each star in the dataset. The photometric measurements are compared to established values to validate the accuracy and consistency of the obtained results.enCopyright 2023 Cindy XiaoProject