82SE    82AS B- DECAY (13.6 S)        2004GA44                  19NDS    201906
 82SE  H TYP=FUL$AUT=J. K. TULI, E. BROWNE$CIT=NDS 157, 260 (2019)$
 82SE2 H CUT=1-Mar-2019$
 82SE c  Based on  XUNDL dataset from 2004Ga44
 82SE2c  Compiled by J. Roediger and B. Singh (McMaster), September 10, 2004
 82SE c  Isotopes of {+82}As were produced via neutron-induced fission of a
 82SE2c  {+235}U target.  The desired isotope was then ionized by plasma
 82SE3c  ionization and mass seperated before being collected on mylar tape in
 82SE4c  front of the detector system.  Tape movements were used in order to
 82SE5c  minimize contributions from possible contaminations by long lived
 82SE6c  nuclides.  In a second experiment of the same reaction, |g-ray
 82SE7c  multi-spectrum scaling was performed where tape movements were
 82SE8c  followed by seven groups of data taken with the beam deflected.
 82SE c  Measured E|g, I|g, |g|g, I|b, |b|g (coin) using standard coaxial HPGe
 82SE2c  detectors, while a Low Energy Photon Ge detector (LEP) was used as a
 82SE3c  |b detector.
 82SE C  Decay scheme is in general agreement with earlier work of
 82SE2C  1975Kr08: 82SE(N,P), fission product, chemical
 82SE3C  separation. Measured EG, IG,GG; GE(LI)
 82SE C  Others:
 82SE C  1970Va31: 82SE(N,P). Measured EB, IB, EG, RI, BG, GG;
 82SE2C  GE(LI) FWHM=3.5 KEV at 1.33 MEV, SI(LI), NAI(TL), and plastic scin.
 82SE C  1970KA04: 82SE(N,P). Measured EG, IG, EB, GG, BG. Measured T1/2(82AS)=
 82SE2C  13.7 S 8 from 342G(T).
 82SE3C  In all experiments both 82AS isotopes are produced. The G's
 82SE2C  of the two decays are separated by 1975Kr08 by comparing the
 82SE3C  relative intensities of sources produced by (N,P) and by
 82SE4C  fission. Intensities are quoted as shown in the drawing
 82SE5C  of 1975Kr08.
 82SE cL E$From least-squares fit to E|g's
 82AS  P 131.6     3  (5-)              13.6 S   4              7489      4
 82AS cP E,T,J$From Adopted Levels
 82AS cP QP$from 2017Wa10
 82SE  N 0.75      8           1
 82SE PN                                                                     3
 82SE CN NR$From 2004Ga44, based on SUMOF (G+CE) TO GS=100 with
 82SE2CN no direct feeding to the GS
 82SE  L 0.0          0+
 82SE  L 654.39    16 2+
 82SE  G 654.4     2  100    5
 82SE  L 1730.03   16 2+
 82SE  B              3      LT             7.1  GT                            ?
 82SES B EAV=2668.6 20
 82SE  G 1075.6    2  12.0   12
 82SE  G 1730.0    2  34     3
 82SE  L 1733.85   21 4+
 82SE  B              5      5              6.8   5                            ?
 82SES B EAV=2666.7 20
 82SE  G 1079.3    2  26     7
 82SE  L 2548.40   19 (3,4+)
 82SE cL J$3 is less likely if J|p(parent)=5-
 82SE  B              20     5             5.93  11
 82SES B EAV=2272.3 20
 82SE  G 814.7     2  15.0   9
 82SE  G 818.3     2  46     2
 82SE  G 1894.2    2  62     3
 82SE  L 2891.78   24  5-
 82SE  B              54     7             5.37   6
 82SES B EAV=2106.2 20
 82SE CB E$EB=3600 200 from BG (1970KA04)
 82SE  G 343.7     2  87     4
 82SE  G 1157.6    2  4.6    5
 82SE  L 3452.3     3 (5-)
 82SE  B              14.4   18            5.70   6                         C
 82SES B EAV=1835.7 20
 82SE cB E$4231 {I19} from |b(560.5|g) coin
 82SE  G 560.5     2  19.2   11
 82SE  L 4088.0     4 (4-,5-)
 82SE  B              7.4    10            5.67   6                         C
 82SES B EAV=1530.0 20
 82SE cB E$3566 {I35} from |b(1539.6|g) coin
 82SE  G 1539.6    3  9.8    8