170W     174OS A DECAY                 1972BE89,1971BO06         18NDS    201811
170W   H TYP=FUL$AUT=C.M. Baglin{+1}, E.A. McCutchan{+2}, S. Basunia{+1$
170W 2 H CIT=NDS 153, 1 (2018)$CUT=1-Oct-2018$
170W  C  1971BO06: sources produced by 164ER(16O,6N), E=90-154 MEV; semi;
170W 2C  measured EA, |a branching.
170W  C  1972BE89: sources produced by 1-GEV proton bombardment of HG targets.
170W  CA IA        Only the 4760A to the GS has been observed. IA for a possible
170W 2CA unobserved 4607A to the 156.9-KEV 2+ state in 170W is estimated to be
170W 3CA less than 11% of ALPHA decay by requiring its hindrance factor
170W 4CA to be greater than 1.0. This does not affect significantly the
170W 5CA computation of the R0 parameter.
170W  CA HF        R0(170W)=1.54 3, assuming HF(4760A)=1.0, T1/2(174OS)=44 S 4
170W 2CA (weighted average of 45 S 5 (1973Be67) and 42 S 6 (1972Be89)),
170W 3CA QA(174OS)=4870 10 (2017WA10) and %A(174OS)=0.020 +10-4 (1971BO06).
174OS  P 0.0         0+                44 S      4              4870      10
170W   N                       0.00020 10
170W  cN BR$from 0.020 {I+10-4} (1971Bo06).
170W   L 0.0         0+
170W   A 4760      10 100      1.0
170W  CA E         measured by 1971BO06.