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Optical observations of SN 2011fe

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arxiv 1311.3484 v1 pith:HUGYPGN2 submitted 2013-11-14 astro-ph.SR

D.Yu.Tsvetkov , S.Yu. Shugarov , I.M. Volkov , V.P. Goranskij , N.N. Pavlyuk , N.A. Katysheva , E.A. Barsukova , A.F. Valeev This is my paper · ORCID
classification astro-ph.SR
keywords curveslightcolourdaysnormalspectrumbandbelongs
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We present UBVRI photometry of the supernova 2011fe in M101, obtained in the interval of 1-652 days after its discovery, as well as one spectrum, taken 105 days after the brightness maximum in the B band. We derived parameters of the light curves, constructed the colour curves and a "quasi-bolometric" light curve. The light curves, colour evolution and spectrum of the object indicate that SN 2011fe belongs to the "normal" subset of type Ia supernovae. It is practically identical to a well-studied "normal" SN Ia 2003du.

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