231RA 231FR B- DECAY (17.6 S) 2001FR05 22NDS 202210
231RA H TYP=FUL$AUT=Balraj Singh, Jagdish K. Tuli, and Edgardo Browne$
231RA2 H CIT=NDS 185, 560 (2022)$CUT=31-Aug-2022$
231RA c 2001Fr05: {+231}Fr was produced by spallation of 1 GeV proton beam on
231RA2c uranium targets. The activity was mass-separated at CERN ISOLDE on-line
231RA3c separator, deposited on a magnetic tape, and then radiations counted at
231RA4c two stations. Measured E|g, I|g, ce, |b|g-, |g|g- and (ce)|g-coin,
231RA5c using HPGe detector for |g rays, plastic scintillators for |b{+-}
231RA6c particles, and a cooled Si(Li) detector with a magnetic mini-orange
231RA8c filter for conversion electrons. Additional measurements were done with
231RA9c the OSIRIS fission product separator in Sweden. See also 2001Bo34
231RAAc from the same lab and group
231RA c 1985Hi02: {+231}Fr produced in spallation reaction of {+238}U induced
231RA2c by 600 MeV protons from the CERN synchrocyclotron, followed by
231RA3c mass-separation using the ISOLDE II online separator. Measured E|g,
231RA4c I|g, x rays, T{-1/2} of {+231}Fr decay. Three |g rays in {+231}Ra
231RA5c were reported, which are listed in comments in this dataset.
231RA c The decay scheme proposed by 2001Fr05 is essentially based on analogy
231RA2c with the structure of N=143 isotone {+233}Th. Evaluators consider the
231RA3c decay scheme to be incomplete in many ways: 1. many |g rays, carrying,
231RA4c significant transition intensities, are unplaced; 2. multipolarities of
231RA5c some of the low-energy transitions, with expected high internal
231RA6c conversion, are not known precisely; 3. with Q value of 3864 keV, the
231RA7c highest proposed level in {+231}Ra is at 1774 keV, which leaves the
231RA8c possibility of either unobserved or unplaced transitions in the decay
231RA9c scheme; 4. several transitions are multiply placed with undivided
231RAAc intensities; 5. the |g|g-coin results are available only in a few
231RABc cases. In this scenario, all the |b feedings and log| {Ift} values
231RACc should be treated as tentative.
231RA cB IB$Deduced by evaluators from |g-ray transition intensity balance.
231RA2cB These values should be considered as only approximate as the decay
231RA3cB scheme is considered incomplete by the evaluators for reasons
231RA4cB mentioned in the header comments
231RA cB LOGFT$All the values should be considered as only approximate since the
231RA2cB decay scheme is considered by the evaluators as incomplete.
231RA cG $Measured I(K x rays)=39 {I4} (1985Hi02) relative to 100 for 432.6-keV
231RA2cG |g ray.
231RA cG E(a)$Tentatively assigned to {+231}Ra.
231RA cG E(b)$Possible doublet.
231RA cG E(c)$Possible multiplet.
231RA cG RI(d)$Contribution from impurities was removed
231RA cG M,MR$From ce data in 2001Fr05. Only the dominant multipolarity is
231RA2cG assigned. Possible admixtures with upper limits are given under
231RA3cG comments. The same assignments are given in the Adopted dataset.
231RA cL E$Deduced from a least-squares fit to |g-ray energies. The gamma rays
231RA2cL with uncertain placements are included in the fitting procedure
231RA cL J$From the Adopted Levels
231RA cL T$From |b|g(t) or |b|g|g(t) for excited states above 80 keV, using
231RA2cL Advanced Time Delayed system (2001Fr05, also 2001Bo34)
231FR P 0.0 (1/2+) 17.6 S 6 3864 14
231FR cP J,T$From {+231}Fr Adopted Levels
231FR cP QP$From 2021Wa16
231RA N 0.25 AP 1.0 1.0
231RA cN NR$Deduced by evaluators, assuming no |b{+-} feeding to g.s. and 46-keV
231RA2cN level, and using summed I(|g+ce)=100% to these levels. Note that
231RA3cN significant I(|g+ce) intensity is unplaced in the decay scheme. In
231RA4cN addition there may be levels above 1775 keV from which transitions
231RA5cN are either not observed or not assigned.
231RA PN 3
231RA G 77.1 3 0.7 3 E1 0.220 4
231RA2 G EL1C+EL2C LE 2.8
231RAS G LC=0.167 3$MC=0.0404 7
231RAS G NC=0.01047 19$OC=0.00226 4$PC=0.000345 6$QC=1.58E-5 3
231RA cG $|d(M2/E1)<0.18
231RA G 82.5 1 1.36 6
231RA G 83.3 1 2.47 9
231RA G 86.2 1 4.1 3 d
231RA G 96.8 3 0.37 8
231RA G 97.5 2 0.70 12 M1 3.35 5 d
231RA2 G EL1C+EL2C=2.3 9 $ EL2C LE 0.82
231RAS G LC=2.54 4$MC=0.607 10
231RAS G NC=0.1600 25$OC=0.0365 6$PC=0.00636 10$QC=0.000500 8
231RA cG $|d(E2/M1)<0.4
231RA G 225.4 2 0.69 13 M1 1.565 22 d
231RA2 G EKC=1.5 5
231RAS G KC=1.259 18$LC=0.232 4$MC=0.0555 8
231RAS G NC=0.01463 21$OC=0.00334 5$PC=0.000582 9$QC=4.56E-5 7
231RA cG $|a(K) exp gives |d(E2/M1)<0.5
231RA G 273.7 2 1.0 2
231RA G 346.5 3 1.2 3 d
231RA2 G EKC LE 0.27
231RA G 400.5 3 0.5 2 b
231RA G 448.1 3 1.7 3
231RA cG $Possible coin. with 88.2-keV x ray
231RA2 G EKC LE 0.17
231RA G 477.9 4 2.4 2 d
231RA cG $Possible coin. with 85.0 and 88.4-keV x ray
231RA2 G EKC LE 0.089
231RA G 492.9 4 2.2 2
231RA cG $Possible coin. with 88.6-keV x ray
231RA G 505.4 4 2.0 2
231RA G 513.6 3 0.73 11 b
231RAF G FLAG=ad
231RA G 542.1 4 0.37 11 a
231RAF G FLAG=d
231RA G 572.7 4 1.5 4
231RA G 617.2 5 3.1 3 d
231RA G 719.6 5 1.1 4 b
231RA G 735.7 4 1.9 5
231RA G 756.2 5 0.6 2
231RA G 770.5 3 2.5 3 b
231RA G 805.7 6 0.67 14
231RA G 818.8 3 1.0 4 b
231RAF G FLAG=a
231RA G 910.9 6 0.57 14 d
231RA G 947.1 5 1.0 2
231RA G 982.2 6 0.9 2 d
231RA G 991.7 6 1.0 2
231RA G 1021.2 5 1.9 4 b
231RA G 1079.8 5 1.4 5 b
231RA G 1126.1 5 0.83 15 b
231RA G 1201.8 5 0.9 5
231RA G 1207.8 5 1.1 3
231RA G 1268.1 5 1.2 2 d
231RA G 1297.1 6 0.7 2
231RA G 1316.7 6 1.1 2
231RA G 1325.8 4 0.9 4 a
231RA G 1468.6 6 2.5 6
231RA G 1558.3 7 0.7 3
231RA G 1583.1 5 5.8 5
231RA G 1609.4 4 0.7 3
231RA G 1653.6 6 0.7 2 b
231RA G 1682.8 6 2.9 5 c
231RA G 1703.6 7 1.5 5
231RA G 1720.7 6 1.1 3
231RA G 1762.3 4 1.2 3
231RA G 1781.9 5 0.9 4
231RA G 1785.9 6 0.6 2
231RA G 1800.7 6 0.9 2 b
231RA G 1802.6 6 1.2 2
231RA G 1828.1 5 0.6 2
231RA G 1839.1 7 1.1 2
231RA G 1856.2 7 0.9 4
231RA G 1870.0 6 1.3 2
231RA G 1876.4 6 1.8 3
231RA G 1965.8 5 0.6 3
231RA G 1973.8 8 0.4 3 a
231RA G 1983.2 11 0.7 2
231RA G 2000.9 7 0.5 2
231RA G 2008.1 6 1.4 2
231RA G 2053.4 8 0.46 14 a
231RA G 2114.8 8 0.49 13
231RA G 2129.3 8 0.6 2 a
231RA G 2133.5 7 0.7 3
231RA G 2206.4 11 0.49 15 d
231RA G 2289.0 8 0.35 13
231RA G 2457.9 8 0.15 5 a
231RA G 2621.3 8 0.13 3 a
231RA L 0.0 (5/2+) 103.9 S 14
231RA cL T$from Adopted Levels
231RA cL J$Nilsson assignment |n5/2[622] to this bandhead is based on the
231RA2cL energy of the |n5/2[622] orbital in {+233}Th. Also on the retardation
231RA3cL of the 66-keV E2 |g ray from the 1/2+, |n1/2[631] state (at 66 keV) to
231RA4cL the 5/2+, |n5/2[622] (ground state).
231RA L 46.23 11 (7/2+)
231RA cL E$level (2001Fr05) in comparison to a low-energy level in N=143
231RA2cL isotone {+233}Th, and from 49.3-keV transition from the 95.5-keV level
231RA cL $Configuration: 7/2+ member of configuration=|n5/2[622]
231RA G 46.3 2 0.27 5 [M1] 29.5 6 ?
231RAS G LC=22.3 5$MC=5.34 11
231RAS G NC=1.41 3$OC=0.322 7$PC=0.0561 11$QC=0.00441 9
231RA L 66.21 9 (1/2+) 53 US AP M
231RA cL J$Nilsson orbital assignment |n1/2[631] to this level is based on the
231RA2cL expected energy of this orbital, and on the systematics of the B(E1)
231RA3cL ratios between |g rays from the 1/2, 1/2[501] state to the 1/2+
231RA4cL and 3/2+ members of the 1/2[631] rotational band in several odd-A
231RA5cL nuclei near {+231}Ra.
231RA cL T$from 66.2|g(t) and K{-|a2} x-ray(t). 2001Fr05 mention that the
231RA2cL half-life is an estimate only, and has significant systematic and
231RA3cL statistical uncertainties
231RA B 31 15 6.2
231RAS B EAV=1475.8 60
231RA cB IB$combined feeding to 66- and 87-keV levels.
231RA G 66.2 1 5.2 2 E2 67.4 10
231RA2 G BE2=0.12 5 (2001Fr05)
231RA2 G EL1C+EL2C=28 4$ EL3C=20 3 $ EMC=14 2$ ENC=4.0 8
231RAS G LC=49.5 8$MC=13.45 22
231RAS G NC=3.55 6$OC=0.753 12$PC=0.1083 17$QC=0.000263 4
231RA cG $|d(E2/M1)>2 or 12.9 {I12}; |DJ|p consistent with pure E2
231RA L 87.64 13 (3/2+)
231RA cL $Configuration: 3/2+ member of |n1/2[631]
231RA G 21.4 0.8 LE[M1] 286 4 S
231RAS G LC=216 3$MC=52.4 8
231RAS G NC=13.82 20$OC=3.15 5$PC=0.550 8$QC=0.0433 6
231RA cG E$|g ray was not observed
231RA L 95.50 9 (5/2-) 4.72 NS 6
231RA cL J$Nilsson orbital assignment |n5/2[572] to this level is based on the
231RA2cL expected energy of this orbital, and on the similarity of B(E1) ratios
231RA3cL between |g rays from the 5/2[752] to the 5/2+ and 7/2+ members of the
231RA4cL 5/2[622] rotational band in {+231}Th and {+229}Ra.
231RA cL T$from |b|g(t). Other: 4.35 ns {I44} from |b|g|g(t)
231RA B 0.6 LT 9.4 GT 1U?
231RAS B EAV=1420.3 60
231RA cB $I|b=0.1 {I5}
231RA G 49.3 1 0.71 4 E1 0.727 10
231RA2 G BE1=3.2E-5 3 (2001Fr05)
231RA2 G EL1C+EL2C LE 9
231RAS G LC=0.549 9$MC=0.1345 21
231RAS G NC=0.0347 6$OC=0.00734 11$PC=0.001061 16$QC=4.16E-5 6
231RA cG $|d(M2/E1)<0.11
231RA cG $Possible coin. with 85.4-keV x ray
231RA G 95.5 1 14.0 10 E1 0.1247 18 C
231RA2 G BE1=8.7E-5 13 (2001Fr05)
231RA cG $E|g=95.6 {I4}, I|g=17 {I3} (1985Hi02), relative to 100 for 432.6|g
231RA2 G EL1C+EL2C LE 0.5 $ EL3C LE 0.15
231RAS G LC=0.0945 14$MC=0.0228 4
231RAS G NC=0.00592 9$OC=0.001289 19$PC=0.000201 3$QC=9.85E-6 14
231RA cG $|d(M2/E1)<0.11
231RA L 285.62 16 (5/2+)
231RA cL J$Nilsson orbital assignment |n5/2[633] to this level is based on the
231RA2cL expected energy of this orbital, and on the similarity of B(M1) ratios
231RA3cL between |g rays from the 5/2[633] to the 5/2+ and 7/2+ members of the
231RA4cL 5/2[622] rotational band in {+233}Th.
231RA B 2.8 3 7.1 ?
231RAS B EAV=1382.6 60
231RA cB IB$|b feeding of 2.8% is unrealistic for |DJ=2, |D|p=no
231RA G 239.4 3 1.1 2 (M1) 1.324 19 & ?
231RAF G FLAG=d
231RA2 G EKC=1.2 3
231RA cG $|a(K)exp for a doubly-placed |g ray
231RAS G KC=1.065 16$LC=0.196 3$MC=0.0469 7
231RAS G NC=0.01236 18$OC=0.00282 4$PC=0.000491 7$QC=3.85E-5 6
231RA cG $|d(E2/M1)<0.45 for a doubly placed |g ray
231RA G 285.7 2 5.8 5 M1 0.811 12 ? ?
231RA2 G EKC=0.71 12 $ EL1C+EL2C=0.10 5
231RAS G KC=0.653 10$LC=0.1199 17$MC=0.0286 4
231RAS G NC=0.00755 11$OC=0.001722 25$PC=0.000300 5$QC=2.35E-5 4
231RA cG $|d(E2/M1)<0.4
231RA L 397.33 13 (3/2+)
231RA cL J$Nilsson orbital assignment |n3/2[631] to this level is based on the
231RA2cL expected energy of this orbital, and on the similarity of B(M1) ratios
231RA3cL between |g rays to members of the 1/2[631] and 5/2[622] rotational
231RA4cL bands
231RA B 3.3 4 7.0
231RAS B EAV=1335.2 60
231RA G 309.9 2 5.1 5 M1 0.648 9
231RA2 G EKC=0.58 11
231RAS G KC=0.522 8$LC=0.0958 14$MC=0.0229 4
231RAS G NC=0.00603 9$OC=0.001375 20$PC=0.000240 4 $QC=1.88E-5 3
231RA cG $|d(E2/M1)<0.35
231RA G 331.2 2 4.5 6 M1 0.540 8 ?
231RA2 G EKC=0.50 15
231RAS G KC=0.435 7$LC=0.0797 12$MC=0.0190 3
231RAS G NC=0.00502 7$OC=0.001144 17$PC=0.000200 3$QC=1.564E-5 22
231RA cG $|d(E2/M1)<0.55
231RA G 397.3 3 1.9 2 (E2(+M1)) 0.7 GT 0.24 18 d
231RA2 G EKC LE 0.18
231RAS G KC=0.19 15$LC=0.040 18$MC=0.010 4
231RAS G NC=0.0025 11$OC=0.00057 25 $PC=0.00010 5 $QC=7E-6 6
231RA cG $|a(K)exp gives E2(+M1) with |d(E2/M1)>0.7 or E1, |DJ|p
231RA2cG favors E2(+M1)
231RA L 455.0 4 (1/2-:9/2-)
231RA B 0.13 3 8.4
231RAS B EAV=1310.7 60
231RA G 359.5 3 0.51 10 dC
231RA L 458.95 16 (1/2-,3/2-) 15 PS LE
231RA cL T$from |b|g|g(t)
231RA B 1.2 2 7.4
231RAS B EAV=1309.1 60
231RA G 363.4 2 4.2 4 M1(+E2) 0.7 7 0.31 11 C
231RA2 G BM1 GE 0.032 (2001Fr05)
231RA2 G EKC=0.24 10
231RAS G KC=0.243 97$LC=0.051 11$MC=0.0124 24
231RAS G NC=0.0033 7$OC=0.00074 15$PC=0.00013 3$QC=8.7E-6 35
231RA G 392.8 3 1.1 4 b ?
231RA2 G BE1 GE 7.2E-5 (2001Fr05)
231RA L 503.33 21 (1/2,3/2,5/2+)
231RA B 0.8 1 7.6
231RAS B EAV=1290.2 60
231RA G 415.6 3 2.6 3 ?
231RA G 437.4 3 1.12 15 &
231RA L 511.36 15 (1/2+,3/2+)
231RA B 1.0 2 7.5
231RAS B EAV=1286.8 60
231RA G 423.8 2 0.7 2 a
231RA G 445.1 2 4.0 4 M1+E2 0.45 30 0.21 4
231RA cG $Possible coin. with 88.2-keV x ray
231RA2 G EKC=0.17 4
231RAS G KC=0.17 4$LC=0.032 4$MC=0.0077 9
231RAS G NC=0.00203 24$OC=0.00046 6$PC=8.0E-5 11$QC=6.0E-6 12
231RA L 520.29 14 (1/2-) 92 PS 5
231RA cL J$Nilsson orbital assignment |n1/2[501] to this level is based on the
231RA2cL characteristic |b{+-} decay pattern between the 1/2[400] (ground state
231RA3cL in {+231}Fr) and 1/2[501] orbitals in several odd-A nuclei near
231RA4cL {+231}Ra. See also arguments for Nilsson orbital assignment to
231RA5cL {+231}Fr ground state.
231RA cL T$from |b|g|g(t)
231RA B 45 3 5.8
231RAS B EAV=1283.1 60
231RA G 123.1 2 0.70 10 E1 0.291 4
231RA2 G BE1=9.8E-6 16 (2001Fr05)
231RA2 G EL1C+EL2C LE 0.38
231RAS G KC=0.227 4$LC=0.0484 7$MC=0.01165 17
231RAS G NC=0.00303 5$OC=0.000665 10$PC=0.0001056 16$QC=5.58E-6 8
231RA cG $|d(M2/E1)<0.17
231RA G 432.6 2 100.0 50 E1 0.0158822 ?
231RA2 G BE1=3.22E-5 21 (2001Fr05)
231RA cG $E|g=432.6 {I2}, I|g=100 {I3} (1985Hi02)
231RA2 G EKC LE 0.022
231RAS G KC=0.01291 19$LC=0.00226 4$MC=0.000535 8
231RAS G NC=0.0001401 20$OC=3.15E-5 5$PC=5.33E-6 8$QC=3.68E-7 6
231RA G 454.0 2 78.1 48 E1 0.0143720 ?
231RA2 G BE1=2.18E-5 15 (2001Fr05)
231RA cG $E|g=454.1 {I2}, I|g=80 {I4} (1985Hi02), relative to 100 for 432.6|g
231RA2 G EKC LE 0.024
231RAS G KC=0.01169 17$LC=0.00203 3$MC=0.000482 7
231RAS G NC=0.0001261 18$OC=2.84E-5 4$PC=4.81E-6 7$QC=3.34E-7 5
231RA L 605.4 3 (1/2-,3/2,5/2+)
231RA B 1.4 3 7.3
231RAS B EAV=1247.0 60
231RA G 510.3 5 1.4 3 C
231RA cG E,RI$from |g|g-coin measurement
231RA G 539.1 3 4.3 9
231RA cG $Possible coin. with 88.2- and 85.4-keV x rays
231RA L 620.59 24 (3/2,5/2,7/2) 12.5 PS LE
231RA cL T$from |b|g|g(t)
231RA B 1.6 2 7.2
231RAS B EAV=1240.6 60
231RA G 525.2 3 6.8 7 C
231RA2 G BM1 GE 0.016 (2001Fr05)
231RA G 620.2 5 1.12 15 d ?
231RA2 G BE1 GE 1.8E-5 (2001Fr05)
231RA L 646.6 4 (1/2-:7/2)
231RA B 0.10 9 8.4 ?
231RAS B EAV=1229.6 60
231RA G 551.3 4 1.3 3 dC
231RA L 740.72 18 (3/2+,5/2+)
231RA B 1.7 3 7.1
231RAS B EAV=1189.7 60
231RA G 645.2 3 1.0 5 ?
231RA G 653.2 3 1.1 3
231RA G 674.6 5 3.0 3 b
231RA G 694.4 4 1.3 7 &
231RA G 740.5 5 0.52 14
231RA L 750.86 18 (1/2,3/2,5/2+)
231RA B 2.4 2 6.9
231RAS B EAV=1185.4 60
231RA G 239.4 3 1.1 2 (M1) & ?
231RA cG M$same assignment of (M1) is given for the doublet
231RA G 353.6 3 0.8 3
231RA G 663.1 3 6.0 6
231RA cG $Possible coin. with 88.6-keV x ray
231RA G 684.6 5 2.7 2 &
231RAF G FLAG=b
231RA L 760.5 4 (1/2,3/2,5/2+)
231RA B 0.5 2 7.6
231RAS B EAV=1181.4 60
231RA G 672.8 5 0.8 2 b
231RA G 694.4 4 1.3 7 &
231RA L 772.80 15 (1/2+,3/2)
231RA B 1.9 3 7.0
231RAS B EAV=1176.2 60
231RA G 252.5 2 0.77 15 ?
231RA G 261.6 3 0.58 11 d
231RA G 375.7 3 0.8 2 &?
231RA G 684.6 5 2.7 2 &
231RA G 706.5 5 2.0 2 c
231RA cG $Possible coin. with 88.2-keV x ray
231RA G 772.8 3 1.8 2 b
231RA L 796.2 3 (1/2,3/2,5/2+)
231RA B 1.0 2 7.3
231RAS B EAV=1166.3 60
231RA G 708.6 5 1.13 15 c
231RA G 730.0 3 2.7 5 b?
231RA L 834.63 18 (1/2+,3/2,5/2-)
231RA B 1.1 2 7.2
231RAS B EAV=1150.0 60
231RA G 314.4 3 0.47 15 ?
231RA G 375.7 3 0.8 2 &?
231RA G 437.4 3 1.12 15 &
231RA G 746.9 4 2.0 4
231RA G 834.5 6 1.3 2 d
231RA L 929.2 4 (1/2,3/2,5/2+)
231RA B 0.2 1 7.9
231RAS B EAV=1110.1 59
231RA G 841.4 6 0.9 2 &
231RAF G FLAG=bd
231RA G 862.9 6 1.4 2 d
231RA L 931.9 3 (1/2,3/2,5/2)
231RA B 0.4 1 7.6
231RAS B EAV=1109.0 59
231RA G 428.8 3 0.5 2 d? ?
231RA G 472.8 5 1.2 3 d
231RA G 843.5 5 0.8 2 b
231RAF G FLAG=d
231RA L 944.31 22 (1/2+,3/2,5/2+)
231RA B 0.9 1 7.3
231RAS B EAV=1103.8 59
231RA G 659.0 5 1.0 2 ? ?
231RA G 877.9 4 0.7 3
231RA G 944.3 3 1.9 3
231RA L 971.1 6 (1/2,3/2,5/2+)
231RA B 0.28 5 7.8
231RAS B EAV=1092.5 59
231RA G 883.6 6 0.56 14 &
231RAF G FLAG=d
231RA G 904.6 10 0.55 14 d
231RA L 1138.79 24 (1/2,3/2,5/2+)
231RA B 0.7 2 7.3
231RAS B EAV=1021.9 59
231RA G 387.7 3 0.55 11 d
231RA G 1051.4 3 1.3 3
231RA G 1072.5 6 1.0 4 &
231RA L 1634.1 4 (1/2,3/2,5/2+)
231RA B 1.0 2 6.8
231RAS B EAV=814.9 58
231RA G 704.8 5 1.5 2 c
231RA G 883.6 6 0.56 14 &
231RA G 1546.4 6 1.1 4
231RA G 1567.8 6 0.8 3
231RA L 1693.3 3 (1/2+,3/2,5/2+)
231RA B 2.0 2 6.4
231RAS B EAV=790.5 58
231RA G 1072.5 6 1.0 4 &
231RA G 1408.0 6 1.0 2 b? ?
231RAF G FLAG=d
231RA G 1605.5 4 3.3 4
231RA G 1627.2 6 1.1 3
231RA G 1693.7 8 1.7 5
231RA L 1718.2 3 (1/2,3/2,5/2+)
231RA B 0.9 1 6.7
231RAS B EAV=780.2 58
231RA G 883.6 6 0.56 14 &
231RA G 1097.8 6 0.7 2
231RA G 1630.6 5 1.9 3
231RA G 1651.9 6 0.5 2 b
231RA L 1730.1 4 (1/2,3/2,5/2+)
231RA B 1.4 2 6.5
231RAS B EAV=775.3 58
231RA G 1642.5 5 3.9 4
231RA G 1663.8 5 1.6 3
231RA L 1773.90 25 (1/2,3/2,5/2+)
231RA B 2.4 4 6.3
231RAS B EAV=757.2 58
231RA G 841.4 6 0.9 2 &
231RA G 939.8 7 0.74 14 d
231RA G 1001.7 6 1.2 10
231RA G 1127.5 5 0.9 2 b
231RA G 1376.1 6 0.9 2 ?
231RA G 1686.1 5 3.8 5 b
231RA G 1707.6 7 1.0 4