The APUS Supernovae Search Program regularly observes about 200 galaxies to search for supernova events. Supernovae are fascinating and vital objects in astronomy because their consistent luminosities serve as "standard candles," enabling accurate measurements from Earth to their host galaxies. They are also the sources for most of the heavy metals in our universe, which have profound implications for life.
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Detecting supernovae requires detailed observations of individual galaxies over extended periods, making this project an ideal candidate for group participation. Recorded images are processed and analyzed using a "blink sequence" method to determine if a supernova is present.