94RU    95PD B+P DECAY (13.3 S)       1982NO06,1982KU15         06NDS    200609
 94RU  H TYP=FUL$AUT=D. Abriola(a), A.A. Sonzogni$CIT=NDS 107, 2423 (2006)$
 94RU2 H CUT=1-Jan-2006$
 94RU C  All information is from 1982No06, except as noted. See
 94RUaC  {+58}Ni({+40}Ca,n2p) in (HI,xn|g) for experimental details
 94RU C  The singles proton spectrum and delayed p|g-coincidence spectrum are
 94RUaC  the  same within statistics indicating that the contamination of the
 94RUaC  proton spectrum by other |b-delayed proton emitters is small and the
 94RUaC  final state in {+94}Ru populated after proton emission is the 2645.
 94RUaC  Feeding of other states in {+94}Ru was not observed by 1982No06
 94RU C  From the prompt p|g-coincidence spectrum, feeding of higher excited
 94RUaC  states is <20% for each of them compared to the feeding of the (8+)
 94RUaC  state
 94RU CL J,T$From adopted levels
 94RU CG E$From p|g-coincidence spectrum. No other |g's were observed by
 94RUaCG 1982No06
 94RU CG RI$From the adopted branching ratios  and I(p)=100 to (8+) state
 94RU CG M$From adopted gammas
 95PD  P 2000      AP(21/2+)           13.3 S    3              5.13E+3   SY
 94RU  N 1.0                   0.0090  16              0.0090 16
 94RU PN                                                                     3
 94RU  L 0           0+                51.8 M    6
 94RU  L 1430.7      2+
 94RU  G 1430.7      100       (E2)                                          C
 94RU  L 2187        4+
 94RU  G 756         100       (E2)                                          C
 94RU  L 2498        6+                65 NS     2
 94RU  G 311.6       97.68     E2                                            C
 94RUS G CC=0.0237$KC=0.02039$LC=0.00270$MC=0.00050
 94RU  L 2645        8+                71 US     4
 94RU  G 146.3       74.91     E2                                            C
 94RUS G CC=0.335$KC=0.277$LC=0.0471$MC=0.00873$NC+=0.00155
 94RU  DP4.5E+3      100                                                     C