151ER    155YB A DECAY (1.793 S)       1996PA01,1979HO10,1991TO0809NDS    200901
151ER  H TYP=FUL$AUT=BALRAJ SINGH$CIT=NDS 110, 1 (2009)$CUT=20-Nov-2008$
151ER c  Others: 1982Bo04, 1980Da09, 1977Ha48, 1964Ma45
151ER c  Source produced in {+109,}{+107}AgI reaction.
151ER c  The parent state T{-1/2} is from 1996Pa01. Others: 1.75~s~{I5}
151ER2c  (1991To08), 1.7~s~{I2} (1982Bo04), 1.59~s~{I22} (1979Ho10), 1.9~s~{I2}
151ER3c  (1977Ha48), 1.8~s~{I3} (1980Da09), 1.65~s~{I15} (1964Ma45)
155YB  P 0.0         (7/2-)            1.793 S   19             5337.6    23
155YB cP $ J|p, T{-1/2} and related comments are mostly from A=155 evaluation
155YB2cP by 2005Re01
155YB cP J$ |a transition, most probably favored, to {+151}Er
155YB2cP (J|p=(7/2-)). The {+155}Yb g.s. is expected to have configuration=(|n
155YB3cP f{-7/2}), since f{-7/2}, the first neutron orbital above the N=82
155YB4cP closed shell, accounts for the g.s. configurations of the even-Z,
155YB5cP odd-N nuclides in this mass region.
155YB cP T$ weighted average of 1.75 s {I5} (1991To08) and 1.800 s {I20}
155YB2cP (1996Pa01). Others: 1.7 s {I2} (1982Bo04); 1.8 s {I3} (1980Da09); 1.59
155YB3cP s {I22} (1979Ho10); 1.9 s {I2} (1977Ha48); and 1.65 s {I15} (1964Ma45).
151ER  N                       0.89    4
151ER cN BR$from weighted average of %|a=84~{I10} (1979Ho10) and 90~{I5}
151ER2cN (1991To08).  %|a deduced (1991To08) from a comparison of |e+|b{++}
151ER3cN branch with that of the 5194|a group and from (1979Ho10) the
151ER4cN intensities of parent and daughter |a lines
151ER  L 0.0         (7/2-)
151ER  A 5200      3 (100)
151ER cA E$weighted average of 5210~{I20} (1964Ma45), 5202~{I10} (1977Ha48),
151ER2cA 5206~{I5} (1979Ho10), 5191~{I5} (1982Bo04), 5202~{I4} (1996Pa01).
151ER3cA Other: 5194 (1991To08)