Sternberg Astronomical Institute Supernova Light Curve Catalogue

SAI Supernova Light Curve Catalogue is the set of U-, B-, V-, Rc-, Ic-, u, g, r, i and z-band light curves of supernovae, discovered up to January 22, 2014. Data include two types of light curves: original and smoothed ones. Original light curves are made of direct observations, while smoothed ones are our fits to true light curves, in which the uncertainties of different observations were excluded.

On the base of this set of light curves, with help of Catalogue's web interface, one can construct color curves of supernovae "on the fly", impose light curves one onto another, draw supernova light curves for observers, specified by user. Also web interface to SAI Supernova Light Curve Catalogue allows to find a nearest observable light curves for user-definited light curves. The latters could be theoretical light curves as well as other observable light curves not included in the Catalogue.

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• Baklanov, P.V., Blinnikov, S.I., Pavlyuk, N.N., Tsvetkov, D.Yu., 2012, in preparation.
• Pavlyuk, N.N., 1998, Pis\'ma v Astron. Zh., 24, P.951
• Pskovskii, Yu. P., 1977, Astronom. Zh., Vol. 54, P. 1188-1201.
• Tsvetkov, D.Yu., 1986, Variable Stars (Peremennye Zvezdy), Volume 22, P.279.
• Tsvetkov, D.Yu., Pavlyuk, N.N., 2010, "Sternberg Astronomical Institute Supernova Light Curve Catalogue", Version May 4, 2010, http://stella.sai.msu.ru/~pavlyuk/snlcurve/
• Tsvetkov, D.Yu., Pavlyuk, N.N., Bartunov, O.S., Pskovskii, Yu.P., 2010, "Sternberg Astronomical Institute Supernova Catalogue", http://www.sai.msu.su/sn/sncat/ .