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Paper detail

Optical observations of SN 2011fe

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.

preprint2013arXivOpen access
D. Yu. TsvetkovS. Yu. ShugarovI. M. VolkovV. P. GoranskijN. N. PavlyukN. A. KatyshevaE. A. BarsukovaA. F. Valeev
astro-ph.SR
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D. Yu. TsvetkovS. Yu. ShugarovI. M. VolkovV. P. GoranskijN. N. PavlyukN. A. KatyshevaE. A. BarsukovaA. F. Valeev

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