52SC    52CA B- DECAY                 1985HU03                  15NDS    201509
 52SC  H TYP=FUL$AUT=YANG DONG, HUO JUNDE$CIT=NDS 128, 185 (2015)$
 52SC2 H CUT=10-Jul-2015$
 52SC c  Sources: produced by the fragmentation of a U target with 600-MeV
 52SC2c  proton beam, on-line mass separation, measured E|g, I|g, |b|g coin,
 52SC3c  Ge(Li) and |b telescope (0.5 mm scintillator sheet).
 52SC cB IB        From |g(+ce) intensity balance at each level.
 52SC cG RI        Photon intensity relative to I|g=100 for the strongest
 52SC2cG transition. Uncertainties deduced from authors' quoted
 52SC3cG uncertainties on I|b's
 52SC cL J         Based on Logft values and shell model calculations.
 52CA  P 0.0          0+                4.6 S     3              5.90E3   14
 52SC  N 0.624     9           1.0       1
 52SC cN NR        calculated by assuming that the intensity of the |b
 52SC2cN transition to the ground state of {+52}Sc (|DJ=3) negligible and
 52SC3cN that the sum of the transition intensities of |g's feeding the g.s.
 52SC4cN is 100%.
 52SC PN                                                                     3
 52SC  L 0.0           3(+)             8.2 S     2
 52SC  L   675.21  23
 52SC  B             5       LT             6.6  GT
 52SCS B EAV=3342 256
 52SC  G 675.2     3 100     2
 52SC  L  1636.43  181+
 52SC  B 4.06E3    2086.8    13            5.07  18
 52SCS B EAV=2870 256
 52SC cB E         from Fermi-Kurie plot analysis of the data (1985Hu03).
 52SC  G 961.2     3 80      2
 52SC  G 1636.4    2 57      1
 52SC  L   2745.7   71+
 52SC  B             11.2    12            5.57  22
 52SCS B EAV=2327 255
 52SC  G 2070.4    6 18      2
 52SC  L   3458.1  10
 52SC  B             0.6     3              6.5   4
 52SCS B EAV=1980 254
 52SC  G 3458.0    101.0     5
 52SC  L   4265.7  151+
 52SC  B             1.4     4              5.8   4
 52SCS B EAV=1588 253
 52SC  G 4265.5    152.2     3