Preliminary CCSN Rate From SDSS-II Supernova Survey

Astronomy and Astrophysics – Astronomy

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Scientific paper

The core collapse supernova rate is measured from SDSS-II data, using a method designed for the results of a rolling survey. First, a type-neutral, total SN rate is calculated based on photometrically selected light curves. The SNIa rate, as measured previously in our survey, is then subtracted from the total rate to find the CCSN rate. This method makes optimal use of our infrastructure for detecting and characterizing SNeIa.

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