SC = ANIKIN 83;
R = NOVO-83-85;
TY = PREP;
D = 1983;
RE = E+ E- --> KS KL;
REC = E+ E- --> KS KL;
BRV = 1.00000;
MODE = EXCL;
MULT = 2;
YN = SIG IN MB;
POINT;
BTM = 1.08800,   1.08800,   1.08800 ECM;
Y = 4.2000E-06, 2.6E-06, 2.1E-06;
POINT.;
BTM = 1.20200,   1.20200,   1.20200 ECM;
Y = 2.3000E-06, 1.4E-06, 1.1E-06;
POINT.;
BTM = 1.30900,   1.27000,   1.34800 ECM;
Y = 1.2000E-07, 1.0E-06, 1.2E-07;
SYS;
SYS-ERR = 10.,10.;
SIG = CORR;
AC = NOVO-VEPP-2M;
DE = CMD;
DS = RPP-2019;
DS. = RPP-2021;
DS. = RAD:B/M;
DSC = Radiative correction includes ISR and 1-loop electron vacuum polarisation term (G. Bonneau, F. Martin, Nucl.Phys. B27 (1971) 381);
DS. = NORM:BHABHA -0.6, 0.6;
DSC = Normalised by the authors to Bhabha e+ e- --> e+ e- cross section with |cos(theta(lab))| < 0.71. The Bhabha cross section was computed using the same Bonneau -- Martin procedure.;
CR = QUESTION: ISR corrections in the signal and Bhabha processes partially are partially canceled.;
SB = ENCODED 24 DEC 2019 BY ZOV;
DS. = EE-2024::FS:ks kl::RAD:b/m -0.6 0.6::WEIGHT:::COMMENT:;
DS. = EE-2025::FS:ks kl::RAD:b/m -0.6 0.6::WEIGHT:::COMMENT:;
DS. = EE-2026::FS:ks kl::RAD:b/m -0.6 0.6::WEIGHT:::COMMENT:;
SB. = UPDATED 07 DEC 2024 BY ZOV;
*E