Detection of Exoplanets Using the Transit Method Open Access
Differential photometry was conducted on the star GSC 3281-0800, a known host to exoplanet HAT-P-32b, using analysis software AstroImageJ. Measurements were plotted from a series of images taken during the transit, via ADU count given from an earth-based digital CCD camera. A definite light curve was established and more details about the properties of this exoplanet were discovered.
Notice to Authors
If you are the author of this work and you have any questions about the information on this page, please use the Contact form to get in touch with us.