UBVRI Photometry of SN 2011fe

  • Lee, Jisoo (CEOU, Astronomy Program, Department of Physics and Astronomy, Seoul National University) ;
  • Im, Myungshin (CEOU, Astronomy Program, Department of Physics and Astronomy, Seoul National University) ;
  • Jeon, Yiseul (CEOU, Astronomy Program, Department of Physics and Astronomy, Seoul National University)
  • 발행 : 2012.10.17

초록

SN 2011fe is the closest and brightest Type Ia supernova in the digital imaging era and thus provides the richest data. We present UBVRI photometry of SN 2011fe for a span of ~180 days after the optical maximum. This paper contains measurements made at SOAO, LOAO, and SNUO and also includes data from a small telescope in Mongolia. We compare the results with the ones obtained by Richmond & Smith (2012) and Vinko et al. (2012).

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