BVRI photometry of the type Ic Hypernova SN 2002ap

Computer Science

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Photometry

Scientific paper

The BVRI photometric observations of type-Ic SN 2002ap at maximum and during the fast-decline phase after maximum are presented. We used our BVRI photometry and published data in order to compute the magnitudes and dates of peak brightness. The absolute magnitude at maximum brightness of SN 2002ap shows that it was fainter than SN 1998bw, but similar to SN 1997ef.

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