The Bulletin of The Korean Astronomical Society (천문학회보)
- Volume 37 Issue 2
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- Pages.86.2-86.2
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- 2012
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- 1226-2692(pISSN)
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)
- Published : 2012.10.17
Abstract
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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