SC = IVANOV 82B;
R = ZETFP 36, 91;
TY = JOUR;
D = 1982;
R. = JETPL 36, 112;
TY = JOUR;
D = 1982;
R. = NOVO-82-50;
TY = PREP;
D = 1982;
RE = E+ E- --> KS KL;
REC = E+ E- --> KS KL;
BRV = 1.00000;
MODE = EXCL;
MULT = 2;
YN = SIG IN MB;
POINT;
BTM = 1.09000,    1.06000,    1.12000 ECM;
Y = 7.0000E-06, 4.1E-06, 3.6E-06;
POINT.;
BTM = 1.16000,    1.12000,    1.20000 ECM;
Y = 4.0000E-06, 3.6E-06, 2.9E-06;
POINT.;
BTM = 1.24000,    1.20000,    1.28000 ECM;
Y = 1.8000E-06, 2.2E-06, 1.6E-06;
POINT.;
BTM = 1.34000,    1.28000,    1.40000 ECM;
Y = 7.0000E-07, 1.3E-06, 7.0E-07;
SYS;
CSYS = Not given;
AC = NOVO-VEPP-2M;
DE = OLYA;
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 -0.71, 0.71;
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 -0.71 0.71::WEIGHT:::COMMENT:;
DS. = EE-2025::FS:ks kl::RAD:b/m -0.71 0.71::WEIGHT:::COMMENT:;
DS. = EE-2026::FS:ks kl::RAD:b/m -0.71 0.71::WEIGHT:::COMMENT:;
SB. = UPDATED 07 DEC 2024 BY ZOV;
*E