Lomonosov Moscow State University, Sternberg Astronomical Institute Supernova Group, Moscow, Russia

Lets Start to Draw a SN Light Curve

Basic Options

Number of SN light curve clusters :
Theoretical model name:		Physical Properties of Models
Shift Theor LC	+Delta(Days) to TH LC	+Delta(Mags) to TH LC

Output Tables

Cluster Id	Members of Cluster
1	1969L_IIP, 1973R_IIP, 1980K_IIL, 1980N_Ia, 1983W_Ia, 1984A_Ia, 1986G_Iaext, 1991T_Iabri, 1998bw_Ic, 1998S_IIn, 2002er_Ia, 2003cg___, 2003kf_Ia, 2004aw_Ic, 2004ek_II, 2004et_II, 2005ki_Ia, 2006gy_IInbr, 2006le_Ia, 2006mp_Ia, 1937C_Ia, 1965N_IIP, 1981B_Ia, 1989B_Ia, 2002hh_II, 2004dj_IIP, 2005hk_Ia, 2007af_Ia, 2007od_II, 2007S_Ia, 2007sr_Ia, 2009bw_IIP, 2009dc_Ia, 2009kn_IIn, 2011bm_Ic, 2011fe_Ia
2	1987A_II, 1991bg_Iaext, 1993J_IIb, 1999gi_II, 2000cb_II, 2002ap_Ic, 2004A_II, 2005ay_II, 2005cs_IIP, 1999em_IIP, 2006X_Ia, 2007gr_Ibc, 2008ax_IIb, 2008bk_II, 2011dh_IIb, 2012hn_I

(C) ITEP-SAI Supernova Study Collaboration. Moscow, Russia. 2006-2016.
(C) Lomonosov Moscow State University, Sternberg Astronomical Institute Supernova Group, Moscow, Russia (MSU, SAI)

Supported by grants of RFBR (13-02-92119), "Scientific Schools of Russia (3458.2010.2)".
(C) Internet site space and support of Alikhanov Institute for Theoretical and Experimental Physics, Moscow, Russia (ITEP)

Calculate Distance Measure between Theoretical and Standard Light Curves:
	Left Boundary: Right Boundary:
Draw light curve of cluster Id members (Id <= Num of clus)
	Add user points: