Type IIn Supernova SN 2010bt photometry
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https://b2find.eudat.eu/dataset/e275fff9-54af-574c-ab93-5b3c8fdab956
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It is well known that massive stars (M>8M_{sun}) evolve up to the collapse of the stellar core, resulting in most cases in a supernova (SN) explosion. Their heterogeneity is...
