Key Features

• Detects exoplanets by spotting periodic dips in star brightness using the transit method.

• Constructs light curves by summing pixel brightness from TESS star videos and plotting trends over time.

• Applies Fourier transform analysis to confirm recurring signals indicative of planetary orbits.

• Produces user-friendly visualizations, including light curves and folded plots, for clear interpretation.

• Enables real-time processing of TESS Target Pixel Files with efficient data handling.