Title:

Analyzing Exoplanet Transits Using Differential Photometry​

Ground-based observations were conducted at the University of New Hampshire's Observatory, and Blue Sky Observatory using differential photometry utilizing AstroImageJ. Light curves were produced for the exoplanet transit of Qatar-1b. These light curves help confirm the existence of the exoplanet and provide verification of key parameters, such as transit depth and planet radius and mid-transit time, as previously measured by other research programs such as Qatar, HAT-P, and TESS.​

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