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Light Curves For Supernova Sn2006jc

Student Name: Daniels, Jonathan
Advisor Name: Moody, J. Ward
Approval Date: 8/1/2008
Report Type: Senior Thesis
Title: Light Curves For Supernova Sn2006jc
Abstract: On October ninth of 2006 a supernova was discovered in the galaxy UGC 4904. It was designated SN 2006jc. This SN is thought to be either a type Ib, a type Ic, or a type Ibc supernova. The progenitor star is thought to have been a Wolf-Rayet star that had a massive eruption two years before the supernova. Alternatively the progenitor may have been a Wolf-Rayet Star in a binary system with the LBV star that had the outburst. We observed this SN for 23 nights from October 26, 2006 to January 3, 2007 using the Tenagra II telescope. These observations were made in V, R, and I filters. We reduced the data and graphed the SN magnitude versus Julian date to make light curves for the three filters. The data obtained and analyzed in this thesis are part of the Swift SN Multi-wavelength Monitoring Project. Based on our light curve we can’t distinguish between type Ib, Ic, or Ibc.
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