171IR    175AU A DECAY (137 MS)        2017Ba46,2011WA37,2010AN0118NDS    201808
171IR  H TYP=FUL$AUT=CORAL M. BAGLIN, E.A. MCCUTCHAN$CIT=NDS 151, 334 (2018)$
171IR2 H CUT=30-Jun-2018$
171IR c  1975Ca06: sources from {+141}Pr({+40}Ca,6n) (E({+40}Ca)=180-290 MeV,
171IR2c  helium-jet transport); measured E|a, I|a
171IR c  1983Sc24: sources from {+92}Mo bombardments of isotopically enriched
171IR2c  targets of rubidium through molybdenum (velocity-filter,
171IR3c  evaporation-residue separation); measured E|a, I|a, T{-1/2}
171IR4c  (position-sensitive silicon surface-barrier detectors).
171IR c  1996Pa01: sources from heavy-ion fusion-evaporation reactions; recoil
171IR2c  mass separator, double-sided Si strip detector (FWHM |< 20 keV);
171IR3c  measured E|a, parent and daughter T{-1/2}, %|a({+171}Ir).
171IR c  2002Ro17: {+175}Au from (11/2-) {+179}Tl |a decay; {+179}Tl produced
171IR2c  by bombardment of 90.4% enriched {+102}Pd targets with {+78}Kr, E=340
171IR3c  MeV (mid-target); gas-filled separator, two parallel-plate avalanche
171IR4c  counters (PPACs), Si strip detector in focal plane, TOF measured
171IR5c  between PPAC and focal plane detector; two HPGe detectors near focal
171IR6c  plane to measure |g and x rays; measured E|a (FWHM=35 keV),
171IR7c  parent-daughter (or granddaughter) correlations; deduced T{-1/2},
171IR8c  corrected for random correlation rates.
171IR c  2010An01: {+175}Au from (11/2-) {+179}Tl |a decay; measured E|g, I|g,
171IR2c  E|a, I|a, T{-1/2}, yield using a single Miniball Ge cluster and a
171IR3c  PSSD.
171IR c  2011Wa37: {+175}Au from {+92}Mo({+86}Sr,p2n) reaction at E=401 MeV; 1
171IR2c  mg/cm{+2} Mg degrader foil; plunger device mounted at target position
171IR3c  of JUROGAM II
171IR c  2017Ba46: {+175}Au source from {+179}Tl |a decay produced in
171IR2c  {+104}Pd({+78}Kr,p2n), with E({+78}Kr)=358 MeV, followed by mass
171IR3c  separation using the RITU separator. Measued E|a, I|a, |a(t) using
171IR4c  two DSSD detectors.
171IR c  Others: 1975Ca06, 1983Sc24, 2001Ko44.
171IR CA HF$R0=1.56 1 (based on R0 for 170OS, 172OS, 170PT, 172PT obtained
171IR2CA from 1998AK04) and assumption that excitations of parent and daughter
171IR3CA states are similar (see comment on 6434|a).
175AU  P 0.0+X        (11/2-)           137 MS    1              6583     4
175AU cP T$weighted average of 136 ms {I1} (2017Ba46), 139 ms {I2} (2011Wa37),
175AU2cP and 138 ms {I5} (2010An01). Others: 143 ms {I8} (2001Ko44), 158 ms
175AU3cP {I3} (2002Ro17),  and 200 ms {I22}, 185 ms {I30} (1996Pa01) (all for
175AU4cP 6434|a).
171IR  N                        0.90   3
171IR cN BR$From (evaporation residue)-|a-|a correlation (2010An01). Other: 94
171IR2cN % {I+6-25} (1983Sc24).
171IR  L 0.0+X        (11/2-)
171IR CL J$from the Adopted Levels.
171IR  A 6434      4 100       2       AP
171IR CA E$weighted average of 6433 {I4} (2017Ba46), 6430 6 (2011WA37, FROM
171IR2CA 2001KO44), 6432 5 (2010AN01), 6438 9 (1996PA01), 6440 10 (1983SC24),
171IR3CA 6440 10 (1975CA06). Were this a GS to GS transition, EA would imply
171IR4CA QA=6585 3, cf. 6583 4 (2017Wa10), SO THE EXCITATIONS OF THE PARENT
171IR5CA AND DAUGHTER STATES MUST BE ALMOST IDENTICAL.
171IR CA E$CORRELATED WITH THE 5920A FROM 171IR (WHICH FEEDS THE 11/2- 92
171IR2CA LEVEL IN 167RE) AND WITH THE 7201A FROM 179TL (2002RO17).