149DY    149HO EC DECAY (56 S)         1994ME13                  22NDS    202210
149DY  H TYP=FUL$AUT=Balraj Singh and Jun Chen$CIT=NDS 185, 2 (2022)$
149DY2 H CUT=23-Aug-2022$
149DY c  1994Me13 (also 1989Me13): {+149}Ho ions were produced via
149DY2c  fusion-evaporation reactions with 5.4 MeV/nucleon {+58}Ni beam on
149DY3c  {+94}Mo and {+95}Mo targets at ISOLDE, GSI, separated by the GSI online
149DY4c  separator and deposited on a transport tape. The |g- and x-rays were
149DY5c  detected with a planar and two coaxial Ge(Li) detectors. Measured E|g,
149DY6c  I|g, I(x-ray), |g|g-coin, |g(x-ray)-coin, |g(t). Deduced levels, J|p,
149DY7c  parent T{-1/2}, conversion coefficients, |g-ray multipolarities, GT
149DY7c  strengths. Comparisons with theoretical calculations. Configurations
149DY8c  are suggested for all levels reported in this decay.
149DY c  Other:
149DY c  1988ToZW: measured T{-1/2} of {+149}Ho isomer:
149DY c  Total decay energy deposit of 6102 keV {I140} calculated by RADLIST
149DY2c  code is in agreement with expected value of 6098 keV {I13}. However
149DY3c  the decay scheme is considered as incomplete since a significant |b
149DY4c  feedings may have missed detection in view of a large gap of about
149DY5c  3 MeV between Q(|e) value and the highest known populated level at 2938
149DY cE TI,LOGFT$I(|e+|b{++}) are from |g intensity balance at each
149DY2cE level. Most of the |b feedings should be treated as upper limits and
149DY3cE correspondingly, the log| {Ift} values as lower limits since the decay
149DY4cE scheme is considered incomplete by the evaluators. Exception is made
149DY5cE for |b feedings for the 1034.6, 1501.0, 2771.0 and 2788.6 level, where
149DY6cE feedings of |>10% can be realistic, and where uncertainties for
149DY7cE log| {Ift} values are given.
149DY cG E,RI$From 1994Me13
149DY cG M,MR$From ce data in 1994Me13, given under comments. The same values
149DY2cG are given in the Adopted Gammas.
149DY cG RI(D)$Estimated from |g|g spectra (1994Me13)
149DY cL E$From a least-squares fit to |g-ray energies
149DY cL J,T$From the Adopted Levels
149HO  P 48.8      2 (1/2+)              56 S    3              6048      13
149HO cP E,J,T$From {+149}Ho Adopted Levels
149HO cP QP$From 2021Wa16
149DY  N  1.0                    1.0      1.0
149DY cN NR$1994Me12 provide photon intensities per 1000 decays, with
149DY2cN statistical uncertainties as well as those from spectral complexity.
149DY3cN Evaluators divide I|g values in 1994Me12 by a factor of 10. Methodology
149DY4cN of measuring absolute |g intensities is not described in 1994Me13
149DY PN                                                                     3
149DY  L 0.0          7/2-              4.2 M    2
149DY  L 1034.6    2  (3/2-)
149DY  E                12   7     5   3   5.5   3                17      9
149DYS E EAV=1839.7 61$CK=0.2283 16$CL=0.03398 24$CM+=0.00997 7
149DY  G 1034.6    2   99.7  20 [E2]                   0.00284 4             C
149DYS G  KC=0.002386 33$LC=0.000352 5$MC=7.75E-5 11
149DYS G  NC=1.785E-5 25$OC=2.57E-6 4$PC=1.377E-7 19
149DY  L 1406.7    3  (1/2+)
149DY  E                 4   4     2   2    5.5  GT               6       6
149DYS E EAV=1666.5 61$CK=0.2781 20$CL=0.0415 3$CM+=0.01217 9
149DY  G 372.1     2    25.3 15 E1                     0.0101714             C
149DYS G  KC=0.00863 12$LC=0.001205 17$MC=0.000263 4
149DYS G  NC=6.04E-5 8$OC=8.66E-6 12$PC=4.63E-7 7
149DY cG  M$|a(K)exp=0.0080 {I16}
149DY  L 1501.0    5  (3/2+)
149DY  E                 8   3    5    2   5.4   2                13      5
149DYS E EAV=1622.8 61$CK=0.2925 21$CL=0.0436 3$CM+=0.01280 9
149DY  G 94.3      3   3.2   12 M1(+E2)  0.7     LT    2.92   10             C
149DYS G  KC=2.21 18$LC=0.56 21$MC=0.13 5
149DYS G  NC=0.029 11$OC=0.0039 13$PC=0.000133 16
149DY cG  M$|a(L)exp=0.59 {I16}
149DY  L 1572.8    4  (3/2+)
149DY  E                 3   1     1   1   5.9                    4       1
149DYS E EAV=1589.5 61$CK=0.3040 22$CL=0.0453 4$CM+=0.01331 10
149DY  G 166.1     2   2.7   5 M1(+E2)   1.5     LT    0.52    4            DC
149DYS G  KC=0.41 7$LC=0.091 21$MC=0.021 5
149DYS G  NC=0.0047 12$OC=0.00064 12$PC=2.4E-5 6
149DY cG  M$|a(K)exp=0.47 {I13}
149DY  L 1626.3    6  (5/2+)
149DY  E                 3   1     1   1   5.9                    4       2    ?
149DYS E EAV=1564.7 61$CK=0.3128 22$CL=0.0467 4$CM+=0.01370 10
149DY cE LOGFT$too low for |DJ=2, |D|p=no transition
149DY  G 591.7     5   3.8   14 (E1)                   0.00356 5            DC
149DYS G  KC=0.00303 4$LC=0.000412 6$MC=8.97E-5 13
149DYS G  NC=2.066E-5 29$OC=2.99E-6 4$PC=1.666E-7 24
149DY cG  M$|a(K)exp<0.005
149DY  L 1727.5    7  (1/2)
149DY  E                 4   1     2   1   5.7                    6       2
149DYS E EAV=1517.9 61$CK=0.3302 23$CL=0.0493 4$CM+=0.01447 11
149DY  G  692.9    6   5.5   14                                             DC
149DY  L 1775.6    6   (1/2)
149DY  E                0.9  6    0.6  4    6.2                   1.5     10
149DYS E EAV=1495.7 60$CK=0.3388 24$CL=0.0506 4$CM+=0.01485 11
149DY  G  741.0    5   1.5   10                                              C
149DY  L 2771.0    7   (1/2+,3/2+)
149DY  E                9    2    19   3   4.5   1                28      5
149DYS E EAV=1040.4 59$CK=0.558 4$CL=0.0838 5$CM+=0.02464 15
149DY  G 1736.4    6   28    5                                              DC
149DY  L 2788.6    6   (1/2+,3/2+)
149DY  E                6    2    13   4   4.7   2                19      6
149DYS E EAV=1032.4 59$CK=0.563 4$CL=0.0845 5$CM+=0.02483 15
149DY  G 1754.0    5   19    6                                              DC
149DY  L 2938.1    6   (1/2+,3/2+)
149DY  E                1.0  3     2   1   5.4                     3      1
149DYS E EAV=964.8 59$CK=0.599 4$CL=0.0902 5$CM+=0.02650 15
149DY  G 1531.4    5    3.0  12                                             DC