150CE    150LA B- DECAY                1995OK02                  13NDS    201306
150CE  H TYP=FUL$AUT=S. K. Basu, A. A. Sonzogni$CIT=NDS 114, 435 (2013)$
150CE2 H CUT=1-Apr-2013$
150CE c  1995Ok02: Source from {+235}U(n,f) thermal. Two Ge detectors and two
150CE2c  plastic scintillators, |b{+-} |g coincidences.
150CE cL J,T$From adopted levels
150CE cB IB$From |g + ce intensity balance.
150CE cG RI$From 1995Ok02
150CE cG M$From adopted gammas
150CE D  CC$ FROM BrIcc v2.2b (20-Jan-2009) 2008Ki07, "Frozen Orbitals" appr.
150LA  P 0.0          (3+)              0.59 S   11              8464     SY
150CE  N 1            1         1         1
150CE cN NR$assuming a) No |b{+-} feeding to g.s.; b) absolute intensity of
150CE2cN 97~keV |g equal to 97.3~{I3} as a result of 2.7% probability of
150CE3cN |b{+-}delayed neutrons.
150CE  L 0.0          0+                4.0 S     6
150CE2 L %B-=100
150CE  L 97.00     10 2+                3.3 NS    8
150CE  G 97.0      1  29.57  9  E2                      2.29
150CES G KC=1.328 19$LC=0.751 11$MC=0.1678 25$NC=0.0359 6$OC=0.00506 8$
150CES G PC=7.01E-5 10$NC+=0.0411 6
150CE  B             68.8    14          5.33    3
150CES B EAV=3414.3
150CE  L 305.70    22 4+                0.26 NS   10
150CE  G 208.7     2  24.6   9  E2                      0.1593
150CES G KC=0.1218 18$LC=0.0295 5$MC=0.00642 10$NC=0.001392 21$OC=0.000206 3$
150CES G PC=7.54E-6 11$NC+=0.001605 24
150CE  B             28.5    10          5.66    3
150CES B EAV=3317.1