ENTRY 23166 20211119 230523166 0 1 SUBENT 23166001 20211119 230523166 1 1 BIB 11 72 23166 1 2 TITLE Neutron activation of natural zinc samples at kT=25 keV23166 1 3 AUTHOR (R.Reifarth,S.Dababneh, M.Heil, F.Kaeppeler, R.Plag, 23166 1 4 K.Sonnabend, E.Uberseder) 23166 1 5 REFERENCE (J,PR/C,85,035802,2012) Data tables. 23166 1 6 #doi:10.1103/PhysRevC.85.035802 23166 1 7 (R,INDC(GER)-0053,2021) Revised values of Karlsruhe 23166 1 8 cross sections. 23166 1 9 INSTITUTE (2GERKFK) F.Kaeppeler 23166 1 10 (2GERFRK) R.Reifarth, R.Plag, K.Sonnabend. 23166 1 11 (3JORJOR) S.Dababneh, 23166 1 12 (2GERGSI) M.Heil 23166 1 13 (1USANOT) E.Uberseder 23166 1 14 REL-REF (I,,M.Heil+,J,PR/C,77,015808,2008) 23166 1 15 Experimental set-up details 23166 1 16 (M,,S.Dababneh+,J,NIM/A,517,230,2004) 23166 1 17 Details of the simulations and the calibration 23166 1 18 procedure of clover detector setup. 23166 1 19 Four references for decay data: 23166 1 20 (R,,E.Browne,J,NDS,111,2425,2010) 23166 1 21 (R,,M.Bhat+,J,NDS,90,269,2000) 23166 1 22 (R,,K.Abusaleem,J,NDS,112,133,2011) 23166 1 23 (R,,X.Huang,J,NDS,110,2533,2009) 23166 1 24 (N,,R.Reifarth+,J,NIM/A,608,139,2009) PINO code. 23166 1 25 (R,12720001,R.L.Macklin,J,NSE,79,265,1981) And private 23166 1 26 communication. 23166 1 27 FACILITY (VDG,2GERKFK) 3.7 MV Van de Graaff accelerator 23166 1 28 METHOD (ACTIV) Four activations with three samples. 23166 1 29 Run Sample Irradiation time Integrated flux x10**13 23166 1 30 I Zn-1 174 min 1.12 +- 0.04 23166 1 31 II Zn-1 2640 min 14.2 +- 0.5 23166 1 32 III Zn-2 1182 min 7.4 +- 0.3 23166 1 33 IV Zn-3 1242 min 4.9 +- 0.3 23166 1 34 INC-SOURCE (P-LI7) Proton beam with an energy of Ep = 1912 keV. 23166 1 35 30 mu-m thick metallic Li layers evaporated onto 23166 1 36 water-cooled copper backings. 23166 1 37 SAMPLE (30-ZN-64,NAT=0.48268) (48.268+-0.214)% 23166 1 38 (30-ZN-68,NAT=0.19024) (19.024+-0.082)% 23166 1 39 (30-ZN-70,NAT=0.00631) (0.631+-0.006)% 23166 1 40 Three metallic natural Zn samples: 23166 1 41 Zn-1 - 409.19 mg, 12 mm diameter; 23166 1 42 Zn-2 - 181.71 mg, 8 mm diameter; 23166 1 43 Zn-3 - 800.72 mg, 12 mm diameter. 23166 1 44 The samples were sandwiched between 0.03 mm thick gold23166 1 45 foils of the same diameter, which served as neutron 23166 1 46 flux monitors. Samples were placed completely inside 23166 1 47 the neutron cone in contact with the neutron target at23166 1 48 the position of highest flux. 23166 1 49 Relative isotope abundance ratios of samples: 23166 1 50 DETECTOR (HPGE) Activities of the gold foils were measured with 23166 1 51 a well calibrated, passively shielded 76 cm3 HPGe 23166 1 52 detector, with 1.7 keV resolution at 1.33 MeV gamma-ray23166 1 53 energy and a relative efficiency of 30%. 23166 1 54 Zn activities were counted with two clover-type HPGe 23166 1 55 detectors facing each other in close geometry. Each 23166 1 56 clover detector (Eurisys Measures) consists of four 23166 1 57 independent n-type Ge crystals in a four-leaf-clover 23166 1 58 arrangement with 0.2 mm gaps in between. The originally23166 1 59 cylindrical crystals of 50 mm diameter, 70 mm length; 23166 1 60 active volume of about 145 cm3 per crystal. 23166 1 61 (GLASD) Neutron flux was continuously monitored and 23166 1 62 recorded in time steps of typically 60 s by means of 23166 1 63 6Li-glass detector at 1 m distance from the target. 23166 1 64 The individual Ge crystals have resolution of typically23166 1 65 2.0 keV at 1.33 MeV. At 122 keV, the peak-to-total 23166 1 66 ratio is about 45 . The efficiency of the clover setup 23166 1 67 was determined with a set of pointlike calibration 23166 1 68 sources (22Na, 54Mn, 60Co, 65Zn, 88Y,131Ba, and 137Cs) 23166 1 69 complemented by a detailed Monte Carlo simulation using23166 1 70 a full model of the setup - see REL-REF of S.Dababneh+.23166 1 71 HISTORY (20120802C) M.M. 23166 1 72 (20211119A) SD: Corrections in all Subents. 23166 1 73 Subents 011-019 added. 23166 1 74 ENDBIB 72 0 23166 1 75 NOCOMMON 0 0 23166 1 76 ENDSUBENT 75 0 23166 199999 SUBENT 23166002 20211119 230523166 2 1 BIB 12 48 23166 2 2 REACTION (30-ZN-64(N,G)30-ZN-65,,SIG,,SPA) 23166 2 3 DECAY-DATA (30-ZN-65,243.93D,DG,1115.539,0.5004) 23166 2 4 HL 243.93+-0.09 d, Egamma 1115.539+-0.002 keV, 23166 2 5 intensity 50.04 +- 0.10 %, from REL-REF of E.Browne. 23166 2 6 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 2 7 MONITOR (79-AU-197(N,G)79-AU-198-G,,SIG,,SPA) 23166 2 8 MONIT-REF (22099002,W.Ratynski+,J,PR/C,37,595,1988) 23166 2 9 DECAY-MON (79-AU-198-G,2.69517D,DG,411.80205,0.9562) 23166 2 10 HL=2.69517+-0.00021 d, Egamma 411.80205+-0.00017 keV, 23166 2 11 intensity 95.62+-0.06 % , from REL-REF of X.Huang. 23166 2 12 ANALYSIS The spectrum-integrated 197Au(n,gamma) cross section 23166 2 13 was obtained by folding the corresponding neutron 23166 2 14 spectra, which were calculated with the code PINO with 23166 2 15 the differential 197Au(n,gamma) cross section of 23166 2 16 R.L.Macklin normalized to the value for kT = 25 keV of 23166 2 17 W.Ratynski (see REL-REFs and MONIT-REF). 23166 2 18 CORRECTION Corrections to the measured peak detection efficiency 23166 2 19 values for the pointlike calibration sources. 23166 2 20 Correction factors compared to ideal pointlike sources 23166 2 21 for the clover setup in single mode: 23166 2 22 Sample Kext Kabs Ksum 23166 2 23 Zn-1 0.9894 0.9877 1.0011 23166 2 24 Zn-2 0.9956 0.9836 1.0006 23166 2 25 Zn-3 0.9884 0.9772 0.9978 23166 2 26 Kext - to the actual diameter of the samples, 23166 2 27 Kabs - to gamma-ray absorption in the sample, 23166 2 28 Ksum - to the possible summing of cascade transitions. 23166 2 29 Gamma detection efficiency - 0.0829 23166 2 30 FLAG (1.) Run I. 23166 2 31 (2.) Run II. 23166 2 32 (3.) Run III. 23166 2 33 (4.) Run IV. 23166 2 34 See details in METHOD and SAMPLE in Subent 001. 23166 2 35 ERR-ANALYS (ERR-1) Uncertainty due to self-absorption. 23166 2 36 (ERR-2) Uncertainty due to detector efficiency. 23166 2 37 (MONIT-ERR) Uncertainty of Au c-s. 23166 2 38 (ERR-3) Uncertainty of Au nuclei number. 23166 2 39 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 2 40 (ERR-5) Uncertainty due to number of Zn-64 nuclei. 23166 2 41 (ERR-6) Uncertainty due to time factors 23166 2 42 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 2 43 (ERR-8) Uncertainty due to time integrated flux. 23166 2 44 (ERR-S) Statistical uncertainty. 23166 2 45 (ERR-T) Total uncertainty 2.8% 23166 2 46 STATUS (TABLE) Tables VII (data), VI (uncertainties) of 23166 2 47 Phys.Rev.,C85(2012)035802 23166 2 48 (SPSDD,23166011) Renormalized. 23166 2 49 HISTORY (20211119A) SD: Subent superseded. 23166 2 50 ENDBIB 48 0 23166 2 51 COMMON 12 6 23166 2 52 KT-DUMMY MONIT MONIT-ERR ERR-1 ERR-2 ERR-3 23166 2 53 ERR-4 ERR-5 ERR-6 ERR-7 ERR-8 ERR-S 23166 2 54 KEV MB PER-CENT PER-CENT PER-CENT PER-CENT 23166 2 55 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 2 56 25. 586. 1.5 0.2 1.5 0.1 23166 2 57 0.06 0.5 0.1 0.2 1.5 0.7 23166 2 58 ENDCOMMON 6 0 23166 2 59 DATA 3 4 23166 2 60 DATA ERR-T FLAG 23166 2 61 MB MB NO-DIM 23166 2 62 54.5 2.1 1. 23166 2 63 54.7 2.2 2. 23166 2 64 52.7 2.2 3. 23166 2 65 52.6 3.0 4. 23166 2 66 ENDDATA 6 0 23166 2 67 ENDSUBENT 66 0 23166 299999 SUBENT 23166003 20211119 230523166 3 1 BIB 6 21 23166 3 2 REACTION (30-ZN-64(N,G)30-ZN-65,,SIG,,SPA) 23166 3 3 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 3 4 ANALYSIS Mean value for four runs. 23166 3 5 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.002 23166 3 6 Because statistical uncertainties were found to 23166 3 7 be practically negligible after averaging the results 23166 3 8 from repeated activations, the final uncertainties are 23166 3 9 determined by systematic effects. 23166 3 10 (ERR-1) Uncertainty due to self-absorption. 23166 3 11 (ERR-2) Uncertainty due to detector efficiency. 23166 3 12 (ERR-3) Uncertainty of Au nuclei number. 23166 3 13 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 3 14 (ERR-5) Uncertainty due to number of Zn-64 nuclei. 23166 3 15 (ERR-6) Uncertainty due to time factors 23166 3 16 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 3 17 (ERR-8) Uncertainty due to time integrated flux. 23166 3 18 STATUS (TABLE) Tables VII (data), VI (uncertainties) of 23166 3 19 Phys.Rev.,C85(2012)035802 23166 3 20 (DEP,23166002) See ANALYSIS. 23166 3 21 (SPSDD,23166012) Renormalized. 23166 3 22 HISTORY (20211119A) SD: Subent superseded. 23166 3 23 ENDBIB 21 0 23166 3 24 COMMON 8 6 23166 3 25 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 3 26 ERR-7 ERR-8 23166 3 27 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 3 28 PER-CENT PER-CENT 23166 3 29 0.2 1.5 0.1 0.06 0.5 0.123166 3 30 0.2 1.5 23166 3 31 ENDCOMMON 6 0 23166 3 32 DATA 3 1 23166 3 33 KT-DUMMY DATA ERR-T 23166 3 34 KEV MB MB 23166 3 35 25. 53.5 1.5 23166 3 36 ENDDATA 3 0 23166 3 37 ENDSUBENT 36 0 23166 399999 SUBENT 23166004 20211119 230523166 4 1 BIB 12 48 23166 4 2 REACTION (30-ZN-68(N,G)30-ZN-69-M,,SIG,,SPA) 23166 4 3 DECAY-DATA (30-ZN-69-M,13.76HR,DG,438.636,0.948) 23166 4 4 HL 13.76+-0.02 h, Egamma 438.636+-0.018 keV, 23166 4 5 intensity 94.8 +- 0.2 %, from REL-REF of M.Bhat+. 23166 4 6 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 4 7 MONITOR (79-AU-197(N,G)79-AU-198-G,,SIG,,SPA) 23166 4 8 DECAY-MON (79-AU-198-G,2.69517D,DG,411.80205,0.9562) 23166 4 9 HL=2.69517+-0.00021 d, Egamma 411.80205+-0.00017 keV, 23166 4 10 intensity 95.62+-0.06 % , from REL-REF of X.Huang. 23166 4 11 MONIT-REF (22099002,W.Ratynski+,J,PR/C,37,595,1988) 23166 4 12 ANALYSIS The spectrum-integrated 197Au(n,gamma) cross section 23166 4 13 was obtained by folding the corresponding neutron 23166 4 14 spectra, which were calculated with the code PINO with 23166 4 15 the differential 197Au(n,gamma) cross section of 23166 4 16 R.L.Macklin normalized to the value for kT = 25 keV of 23166 4 17 W.Ratynski (see REL-REFs and MONIT-REF). 23166 4 18 CORRECTION Corrections to the measured peak detection efficiency 23166 4 19 values for the pointlike calibration sources. 23166 4 20 Correction factors compared to ideal pointlike sources 23166 4 21 for the clover setup in single mode: 23166 4 22 Sample Kext Kabs Ksum 23166 4 23 Zn-1 0.9901 0.9794 0.999 23166 4 24 Zn-2 0.9938 0.9783 0.9991 23166 4 25 Zn-3 0.9906 0.9592 0.9994 23166 4 26 Kext - to the actual diameter of the samples, 23166 4 27 Kabs - to gamma-ray absorption in the sample, 23166 4 28 Ksum - to the possible summing of cascade transitions. 23166 4 29 Gamma detection efficiency - 0.1863 23166 4 30 FLAG (1.) Run I. 23166 4 31 (2.) Run II. 23166 4 32 (3.) Run III. 23166 4 33 (4.) Run IV. 23166 4 34 See details in METHOD and SAMPLE in Subent 001. 23166 4 35 ERR-ANALYS (ERR-1) Uncertainty due to self-absorption. 23166 4 36 (ERR-2) Uncertainty due to detector efficiency. 23166 4 37 (MONIT-ERR) Uncertainty of Au c-s. 23166 4 38 (ERR-3) Uncertainty of Au nuclei number. 23166 4 39 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 4 40 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 4 41 (ERR-6) Uncertainty due to time factors . 23166 4 42 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 4 43 (ERR-8) Uncertainty due to time integrated flux. 23166 4 44 (ERR-S) Statistical uncertainty. 23166 4 45 (ERR-T) Total uncertainty 2.8% 23166 4 46 STATUS (TABLE) Tables VII (data), VI (uncertainties) of 23166 4 47 Phys.Rev.,C85(2012)035802 23166 4 48 (SPSDD,23166013) Renormalized. 23166 4 49 HISTORY (20211119A) SD: Subent superseded. 23166 4 50 ENDBIB 48 0 23166 4 51 COMMON 12 6 23166 4 52 KT-DUMMY MONIT MONIT-ERR ERR-1 ERR-2 ERR-3 23166 4 53 ERR-4 ERR-5 ERR-6 ERR-7 ERR-8 ERR-S 23166 4 54 KEV MB PER-CENT PER-CENT PER-CENT PER-CENT 23166 4 55 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 4 56 25. 586. 1.5 0.2 1.5 0.1 23166 4 57 0.06 0.4 0.2 0.2 1.5 0.9 23166 4 58 ENDCOMMON 6 0 23166 4 59 DATA 3 4 23166 4 60 DATA ERR-T FLAG 23166 4 61 MB MB NO-DIM 23166 4 62 3.27 0.13 1. 23166 4 63 3.38 0.14 2. 23166 4 64 3.25 0.14 3. 23166 4 65 3.31 0.19 4. 23166 4 66 ENDDATA 6 0 23166 4 67 ENDSUBENT 66 0 23166 499999 SUBENT 23166005 20211119 230523166 5 1 BIB 6 21 23166 5 2 REACTION (30-ZN-68(N,G)30-ZN-69-M,,SIG,,SPA) 23166 5 3 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 5 4 ANALYSIS Mean value for four runs. 23166 5 5 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.004 23166 5 6 Because statistical uncertainties were found to 23166 5 7 be practically negligible after averaging the results 23166 5 8 from repeated activations, the final uncertainties are 23166 5 9 determined by systematic effects. 23166 5 10 (ERR-1) Uncertainty due to self-absorption. 23166 5 11 (ERR-2) Uncertainty due to detector efficiency. 23166 5 12 (ERR-3) Uncertainty of Au nuclei number. 23166 5 13 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 5 14 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 5 15 (ERR-6) Uncertainty due to time factors . 23166 5 16 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 5 17 (ERR-8) Uncertainty due to time integrated flux. 23166 5 18 STATUS (TABLE) Tables VII (data), VI (uncertainties) of 23166 5 19 Phys.Rev.,C85(2012)035802 23166 5 20 (DEP,23166004) See ANALYSIS. 23166 5 21 (SPSDD,23166014) Renormalized. 23166 5 22 HISTORY (20211119A) SD: Subent superseded. 23166 5 23 ENDBIB 21 0 23166 5 24 COMMON 8 6 23166 5 25 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 5 26 ERR-7 ERR-8 23166 5 27 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 5 28 PER-CENT PER-CENT 23166 5 29 0.2 1.5 0.1 0.06 0.4 0.223166 5 30 0.2 1.5 23166 5 31 ENDCOMMON 6 0 23166 5 32 DATA 3 1 23166 5 33 KT-DUMMY DATA ERR-T 23166 5 34 KEV MB MB 23166 5 35 25. 3.30 0.09 23166 5 36 ENDDATA 3 0 23166 5 37 ENDSUBENT 36 0 23166 599999 SUBENT 23166006 20211119 230523166 6 1 BIB 13 55 23166 6 2 REACTION (30-ZN-70(N,G)30-ZN-71-M,,SIG,,SPA) 23166 6 3 DECAY-DATA (30-ZN-71-M,3.96HR,DG,487.30,0.612) 23166 6 4 HL 3.96+-0.05 h, Egamma 487.30 +- 0.04 keV, 23166 6 5 intensity 61.2 +- 2.3 %, from REL-REF of K.Abusaleem. 23166 6 6 See also ADD-RES for HL measured in this experiment. 23166 6 7 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 6 8 MONITOR (79-AU-197(N,G)79-AU-198-G,,SIG,,SPA) 23166 6 9 DECAY-MON (79-AU-198-G,2.69517D,DG,411.80205,0.9562) 23166 6 10 HL=2.69517+-0.00021 d, Egamma 411.80205+-0.00017 keV, 23166 6 11 intensity 95.62+-0.06 % , from REL-REF of X.Huang. 23166 6 12 MONIT-REF (22099002,W.Ratynski+,J,PR/C,37,595,1988) 23166 6 13 ANALYSIS The spectrum-integrated 197Au(n,gamma) cross section 23166 6 14 was obtained by folding the corresponding neutron 23166 6 15 spectra, which were calculated with the code PINO with 23166 6 16 the differential 197Au(n,gamma) cross section of 23166 6 17 R.L.Macklin normalized to the value for kT = 25 keV of 23166 6 18 W.Ratynski (see REL-REFs and MONIT-REF). 23166 6 19 ADD-RES (DECAY) New value of Zn-71-m HL was measured in this 23166 6 20 work from the decay curves of three (386, 487, 620 keV)23166 6 21 gamma transitions in 71Ga to be 4.125 +-0.007 h. 23166 6 22 Combining this new result with the values of previous 23166 6 23 measurements, weighted average of 4.120+-0.007 h was 23166 6 24 obtained. 23166 6 25 CORRECTION Corrections to the measured peak detection efficiency 23166 6 26 values for the pointlike calibration sources. 23166 6 27 Correction factors compared to ideal pointlike sources 23166 6 28 for the clover setup in single mode: 23166 6 29 Sample Kext Kabs Ksum 23166 6 30 Zn-1 0.9894 0.9877 1.0011 23166 6 31 Zn-2 0.9956 0.9836 1.0006 23166 6 32 Zn-3 0.9884 0.9772 0.9978 23166 6 33 Kext - to the actual diameter of the samples, 23166 6 34 Kabs - to gamma-ray absorption in the sample, 23166 6 35 Ksum - to the possible summing of cascade transitions. 23166 6 36 Gamma detection efficiency - 0.0829 . 23166 6 37 FLAG (1.) Run I. 23166 6 38 (2.) Run II. 23166 6 39 (3.) Run III. 23166 6 40 (4.) Run IV. 23166 6 41 See details in METHOD and SAMPLE in Subent 001. 23166 6 42 ERR-ANALYS (ERR-1) Uncertainty due to self-absorption. 23166 6 43 (ERR-2) Uncertainty due to detector efficiency. 23166 6 44 (MONIT-ERR) Uncertainty of Au c-s. 23166 6 45 (ERR-3) Uncertainty of Au nuclei number. 23166 6 46 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 6 47 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 6 48 (ERR-6) Uncertainty due to time factors . 23166 6 49 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 6 50 (ERR-8) Uncertainty due to time integrated flux. 23166 6 51 (ERR-S) Statistical uncertainty. 23166 6 52 (ERR-T) Total uncertainty 5.1 % . 23166 6 53 STATUS (TABLE) Tables VII (data), VI (uncertainties) of 23166 6 54 Phys.Rev.,C85(2012)035802 23166 6 55 (SPSDD,23166015) Renormalized. 23166 6 56 HISTORY (20211119A) SD: Subent superseded. 23166 6 57 ENDBIB 55 0 23166 6 58 COMMON 12 6 23166 6 59 KT-DUMMY MONIT MONIT-ERR ERR-1 ERR-2 ERR-3 23166 6 60 ERR-4 ERR-5 ERR-6 ERR-7 ERR-8 ERR-S 23166 6 61 KEV MB PER-CENT PER-CENT PER-CENT PER-CENT 23166 6 62 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 6 63 25. 586. 1.5 0.2 1.5 0.1 23166 6 64 0.06 0.9 1.3 3.8 2.4 0.8 23166 6 65 ENDCOMMON 6 0 23166 6 66 DATA 3 4 23166 6 67 DATA ERR-T FLAG 23166 6 68 MB MB NO-DIM 23166 6 69 6.69 0.40 1. 23166 6 70 7.46 0.43 2. 23166 6 71 6.39 0.37 3. 23166 6 72 6.75 0.47 4. 23166 6 73 ENDDATA 6 0 23166 6 74 ENDSUBENT 73 0 23166 699999 SUBENT 23166007 20211119 230523166 7 1 BIB 6 21 23166 7 2 REACTION (30-ZN-70(N,G)30-ZN-71-M,,SIG,,SPA) 23166 7 3 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 7 4 ANALYSIS Mean value for four runs. 23166 7 5 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.006 23166 7 6 Because statistical uncertainties were found to 23166 7 7 be practically negligible after averaging the results 23166 7 8 from repeated activations, the final uncertainties are 23166 7 9 determined by systematic effects. 23166 7 10 (ERR-1) Uncertainty due to self-absorption. 23166 7 11 (ERR-2) Uncertainty due to detector efficiency. 23166 7 12 (ERR-3) Uncertainty of Au nuclei number. 23166 7 13 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 7 14 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 7 15 (ERR-6) Uncertainty due to time factors . 23166 7 16 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 7 17 (ERR-8) Uncertainty due to time integrated flux. 23166 7 18 STATUS (TABLE) Tables VII (data), VI (uncertainties) of 23166 7 19 Phys.Rev.,C85(2012)035802 23166 7 20 (DEP,23166006) See ANALYSIS. 23166 7 21 (SPSDD,23166016) Renormalized. 23166 7 22 HISTORY (20211119A) SD: Subent superseded. 23166 7 23 ENDBIB 21 0 23166 7 24 COMMON 8 6 23166 7 25 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 7 26 ERR-7 ERR-8 23166 7 27 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 7 28 PER-CENT PER-CENT 23166 7 29 0.2 1.5 0.1 0.06 0.9 1.323166 7 30 3.8 2.4 23166 7 31 ENDCOMMON 6 0 23166 7 32 DATA 3 1 23166 7 33 KT-DUMMY DATA ERR-T 23166 7 34 KEV MB MB 23166 7 35 25. 6.79 0.34 23166 7 36 ENDDATA 3 0 23166 7 37 ENDSUBENT 36 0 23166 799999 SUBENT 23166008 20211119 230523166 8 1 BIB 11 42 23166 8 2 REACTION (30-ZN-70(N,G)30-ZN-71-G,,SIG,,SPA) 23166 8 3 Only run I 23166 8 4 DECAY-DATA (30-ZN-71-G,2.45MIN,DG,910.3,0.0784) 23166 8 5 HL=2.45+-0.10 min, Egamma 910.3 +-0.1 keV, 23166 8 6 intensity 7.84 +- 0.64 %, from REL-REF of K.Abusaleem 23166 8 7 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 8 8 MONITOR (79-AU-197(N,G)79-AU-198-G,,SIG,,SPA) 23166 8 9 DECAY-MON (79-AU-198-G,2.69517D,DG,411.80205,0.9562) 23166 8 10 HL=2.69517+-0.00021 D, Egamma 411.80205+-0.00017 keV, 23166 8 11 intensity 95.62+-0.06 % , from REL-REF of X.Huang. 23166 8 12 MONIT-REF (22099002,W.Ratynski+,J,PR/C,37,595,1988) 23166 8 13 ANALYSIS The spectrum-integrated 197Au(n,gamma) cross section 23166 8 14 was obtained by folding the corresponding neutron 23166 8 15 spectra, which were calculated with the code PINO with 23166 8 16 the differential 197Au(n,gamma) cross section of 23166 8 17 R.L.Macklin normalized to the value for kT = 25 keV of 23166 8 18 W.Ratynski (see REL-REFs and MONIT-REF). 23166 8 19 CORRECTION Corrections to the measured peak detection efficiency 23166 8 20 values for the pointlike calibration sources. 23166 8 21 Correction factors compared to ideal pointlike sources 23166 8 22 for the clover setup in single mode: 23166 8 23 Sample Kext Kabs Ksum 23166 8 24 Zn-1 0.9955 0.9847 0.963 23166 8 25 Kext - to the actual diameter of the samples, 23166 8 26 Kabs - to gamma-ray absorption in the sample, 23166 8 27 Ksum - to the possible summing of cascade transitions. 23166 8 28 Gamma detection efficiency - 0.1547 23166 8 29 ERR-ANALYS (ERR-1) Uncertainty due to self-absorption. 23166 8 30 (ERR-2) Uncertainty due to detector efficiency. 23166 8 31 (MONIT-ERR) Uncertainty of Au c-s. 23166 8 32 (ERR-3) Uncertainty of Au nuclei number. 23166 8 33 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 8 34 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 8 35 (ERR-6) Uncertainty due to time factors . 23166 8 36 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 8 37 (ERR-8) Uncertainty due to time integrated flux. 23166 8 38 (ERR-S) Statistical uncertainty. 23166 8 39 (ERR-T) Total uncertainty 16.% 23166 8 40 STATUS (TABLE) Tables VII (data), VI (uncertainties) of 23166 8 41 Phys.Rev.,C85(2012)035802 23166 8 42 (SPSDD,23166017) Renormalized. 23166 8 43 HISTORY (20211119A) SD: Subent superseded. 23166 8 44 ENDBIB 42 0 23166 8 45 COMMON 11 6 23166 8 46 MONIT MONIT-ERR ERR-1 ERR-2 ERR-3 ERR-4 23166 8 47 ERR-5 ERR-6 ERR-7 ERR-8 ERR-S 23166 8 48 MB PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 8 49 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 8 50 586. 1.5 0.2 1.5 0.1 0.0623166 8 51 0.9 4.0 8.2 2.5 13. 23166 8 52 ENDCOMMON 6 0 23166 8 53 DATA 3 1 23166 8 54 KT-DUMMY DATA ERR-T 23166 8 55 KEV MB MB 23166 8 56 25. 4.18 0.67 23166 8 57 ENDDATA 3 0 23166 8 58 ENDSUBENT 57 0 23166 899999 SUBENT 23166009 20211119 230523166 9 1 BIB 8 33 23166 9 2 REACTION (30-ZN-64(N,G)30-ZN-65,,SIG,,MXW,DERIV) 23166 9 3 ADD-RES Normalization to the present results for kT = 25 keV 23166 9 4 was done, using data of Z.Y.Bao+: 23166 9 5 KT,keV MACS,mb 23166 9 6 5. 123. 23166 9 7 10. 95.9 23166 9 8 15. 78.2 23166 9 9 20. 66.6 23166 9 10 25. 58.6 +- 1.7 23166 9 11 30. 52.4 +- 1.7 23166 9 12 40. 46.2 23166 9 13 50. 41.7 23166 9 14 60. 39.1 23166 9 15 80. 35.5 23166 9 16 100. 33.7 23166 9 17 REL-REF (R,,Z.Y.Bao+,J,AND,76,70,2000) 23166 9 18 ANALYSIS Data were derived from measure c-s - see CORRECTION. 23166 9 19 CORRECTION Correction was done for pure Maxwellian spectrum taking23166 9 20 into account cutoff at 106 keV; corrections are between23166 9 21 3% and 5%. 23166 9 22 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.003 23166 9 23 (ERR-1) Uncertainty due to self-absorption. 23166 9 24 (ERR-2) Uncertainty due to detector efficiency. 23166 9 25 (ERR-3) Uncertainty of Au nuclei number. 23166 9 26 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 9 27 (ERR-5) Uncertainty due to number of Zn-64 nuclei. 23166 9 28 (ERR-6) Uncertainty due to time factors 23166 9 29 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 9 30 (ERR-8) Uncertainty due to time integrated flux. 23166 9 31 STATUS (TABLE) Table VIII of Phys.Rev.,C85(2012)035802 23166 9 32 (DEP,23166003) 23166 9 33 (SPSDD,23166018) Renormalized. 23166 9 34 HISTORY (20211119A) SD: Subent superseded. 23166 9 35 ENDBIB 33 0 23166 9 36 COMMON 8 6 23166 9 37 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 9 38 ERR-7 ERR-8 23166 9 39 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 9 40 PER-CENT PER-CENT 23166 9 41 0.2 1.5 0.1 0.06 0.5 0.123166 9 42 0.2 1.5 23166 9 43 ENDCOMMON 6 0 23166 9 44 DATA 3 1 23166 9 45 KT DATA ERR-T 23166 9 46 KEV MB MB 23166 9 47 25. 58.6 1.7 23166 9 48 ENDDATA 3 0 23166 9 49 ENDSUBENT 48 0 23166 999999 SUBENT 23166010 20211119 230523166 10 1 BIB 8 29 23166 10 2 REACTION (30-ZN-70(N,G)30-ZN-71,,SIG,,MXW,DERIV) 23166 10 3 ADD-RES Normalization to the present results for kT = 25 keV 23166 10 4 was done, using data of Z.Y.Bao+: 23166 10 5 5. 28.4 23166 10 6 10. 18.9 23166 10 7 15. 14.9 23166 10 8 20. 13.1 23166 10 9 25. 11.7 +- 0.8 23166 10 10 30. 10.7 +- 0.8 23166 10 11 40. 9.3 23166 10 12 50. 8.4 23166 10 13 60. 7.7 23166 10 14 80. 6.8 23166 10 15 100. 6.2 23166 10 16 REL-REF (R,,Z.Y.Bao+,J,AND,76,70,2000) 23166 10 17 ANALYSIS Data were derived from measure c-s - see CORRECTION. 23166 10 18 CORRECTION Correction was done for pure Maxwellian spectrum taking23166 10 19 into account cutoff at 106 keV; corrections are between23166 10 20 3% and 5%. 23166 10 21 ERR-ANALYS (ERR-T) Error propagation is given in Subents 007,008 23166 10 22 (ERR-1) Uncertainty due to self-absorption. 23166 10 23 (ERR-2) Uncertainty due to detector efficiency. 23166 10 24 (ERR-3) Uncertainty of Au nuclei number. 23166 10 25 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 10 26 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 10 27 STATUS (TABLE) Table VIII of Phys.Rev.,C85(2012)035802 23166 10 28 (DEP,23166007) 23166 10 29 (DEP,23166008) 23166 10 30 HISTORY (20211119C) SD 23166 10 31 ENDBIB 29 0 23166 10 32 COMMON 5 3 23166 10 33 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 23166 10 34 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 10 35 0.2 1.5 0.1 0.06 0.9 23166 10 36 ENDCOMMON 3 0 23166 10 37 DATA 3 1 23166 10 38 KT DATA ERR-T 23166 10 39 KEV MB MB 23166 10 40 25. 11.7 0.8 23166 10 41 ENDDATA 3 0 23166 10 42 ENDSUBENT 41 0 23166 1099999 SUBENT 23166011 20211119 230523166 11 1 BIB 12 29 23166 11 2 REACTION (30-ZN-64(N,G)30-ZN-65,,SIG,,SPA) 23166 11 3 DECAY-DATA (30-ZN-65,243.93D,DG,1115.539,0.5004) 23166 11 4 HL 243.93+-0.09 d, Egamma 1115.539+-0.002 keV, 23166 11 5 intensity 50.04 +- 0.10 %, from REL-REF of E.Browne. 23166 11 6 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 11 7 MONITOR (79-AU-197(N,G)79-AU-198-G,,SIG,,SPA) 23166 11 8 DECAY-MON (79-AU-198-G,3881.0MIN,DG,411.80,0.9558) 23166 11 9 MONIT-REF (,R.Reifarth+,J,EPJ/P,133,424,2018) 23166 11 10 ANALYSIS Cross section value in Subent 23166.002 is 23166 11 11 renormalized for new gold cross section. 23166 11 12 Measured quantity at kT=25 keV: cross section ratio 23166 11 13 64Zn/197Au = 0.0915+-0.0040 23166 11 14 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 11 15 FLAG (1.) Run I. 23166 11 16 (2.) Run II. 23166 11 17 (3.) Run III. 23166 11 18 (4.) Run IV. 23166 11 19 See details in METHOD and SAMPLE in Subent 001. 23166 11 20 ERR-ANALYS (ERR-1) Uncertainty due to self-absorption. 23166 11 21 (ERR-2) Uncertainty due to detector efficiency. 23166 11 22 (MONIT-ERR) Uncertainty of Au c-s. 23166 11 23 (ERR-5) Uncertainty due to number of Zn-64 nuclei. 23166 11 24 (ERR-6) Uncertainty due to time factors . 23166 11 25 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 11 26 (ERR-8) Uncertainty due to time integrated flux. 23166 11 27 (ERR-S) Statistical uncertainty. 23166 11 28 (ERR-T) Total uncertainty 23166 11 29 STATUS (TABLE) Table on p.339 of INDC(GER)-0053 23166 11 30 HISTORY (20211119C) SD 23166 11 31 ENDBIB 29 0 23166 11 32 COMMON 10 6 23166 11 33 KT-DUMMY MONIT MONIT-ERR ERR-1 ERR-2 ERR-5 23166 11 34 ERR-6 ERR-7 ERR-8 ERR-S 23166 11 35 KEV MB PER-CENT PER-CENT PER-CENT PER-CENT 23166 11 36 PER-CENT PER-CENT PER-CENT PER-CENT 23166 11 37 25. 622.7 1.0 0.2 1.5 0.523166 11 38 0.1 0.2 1.5 0.7 23166 11 39 ENDCOMMON 6 0 23166 11 40 DATA 3 4 23166 11 41 DATA ERR-T FLAG 23166 11 42 MB MB NO-DIM 23166 11 43 57.9 2.1 1. 23166 11 44 58.1 2.2 2. 23166 11 45 56.0 2.3 3. 23166 11 46 55.9 3.1 4. 23166 11 47 ENDDATA 6 0 23166 11 48 ENDSUBENT 47 0 23166 1199999 SUBENT 23166012 20211119 230523166 12 1 BIB 7 24 23166 12 2 REACTION 1((30-ZN-64(N,G)30-ZN-65,,SIG,,SPA)/ 23166 12 3 (79-AU-197(N,G)79-AU-198,,SIG,,SPA)) 23166 12 4 2(30-ZN-64(N,G)30-ZN-65,,SIG,,SPA) 23166 12 5 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 12 6 ANALYSIS Mean value for four runs. 23166 12 7 Cross section value in Subent 23166.003 is 23166 12 8 renormalized for new gold cross section 23166 12 9 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 12 10 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.003 23166 12 11 Because statistical uncertainties were found to 23166 12 12 be practically negligible after averaging the results 23166 12 13 from repeated activations, the final uncertainties are 23166 12 14 determined by systematic effects. 23166 12 15 (ERR-1) Uncertainty due to self-absorption. 23166 12 16 (ERR-2) Uncertainty due to detector efficiency. 23166 12 17 (ERR-3) Uncertainty of Au nuclei number. 23166 12 18 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 12 19 (ERR-5) Uncertainty due to number of Zn-64 nuclei. 23166 12 20 (ERR-6) Uncertainty due to time factors 23166 12 21 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 12 22 (ERR-8) Uncertainty due to time integrated flux. 23166 12 23 STATUS (TABLE) Table on p.340 of INDC(GER)-0053 23166 12 24 (DEP,23166002) See ANALYSIS. 23166 12 25 HISTORY (20211119C) SD 23166 12 26 ENDBIB 24 0 23166 12 27 COMMON 8 6 23166 12 28 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 12 29 ERR-7 ERR-8 23166 12 30 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 12 31 PER-CENT PER-CENT 23166 12 32 0.2 1.5 0.1 0.06 0.5 0.123166 12 33 0.2 1.5 23166 12 34 ENDCOMMON 6 0 23166 12 35 DATA 5 1 23166 12 36 KT-DUMMY DATA 1ERR-T 1DATA 2ERR-T 2 23166 12 37 KEV NO-DIM NO-DIM MB MB 23166 12 38 25. 0.0913 0.0026 56.8 1.5 23166 12 39 ENDDATA 3 0 23166 12 40 ENDSUBENT 39 0 23166 1299999 SUBENT 23166013 20211119 230523166 13 1 BIB 12 29 23166 13 2 REACTION (30-ZN-68(N,G)30-ZN-69-M,,SIG,,SPA) 23166 13 3 DECAY-DATA (30-ZN-69-M,13.76HR,DG,438.636,0.948) 23166 13 4 HL=13.76+-0.02 h, Egamma 438.636+-0.018 keV, 23166 13 5 intensity 94.8 +- 0.2 %, from REL-REF of M.Bhat+. 23166 13 6 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 13 7 MONITOR (79-AU-197(N,G)79-AU-198-G,,SIG,,SPA) 23166 13 8 DECAY-MON (79-AU-198-G,3881.0MIN,DG,411.80,0.9558) 23166 13 9 MONIT-REF (,R.Reifarth+,J,EPJ/P,133,424,2018) 23166 13 10 ANALYSIS Cross section value in Subent 23166.004 is 23166 13 11 renormalized for new gold cross section 23166 13 12 Measured quantity at kT=25 keV: cross section ratio 23166 13 13 (68Zn(ng)68Zn-m)/197Au = 0.00583+-0.0026 23166 13 14 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 13 15 FLAG (1.) Run I. 23166 13 16 (2.) Run II. 23166 13 17 (3.) Run III. 23166 13 18 (4.) Run IV. 23166 13 19 See details in METHOD and SAMPLE in Subent 001. 23166 13 20 ERR-ANALYS (ERR-1) Uncertainty due to self-absorption. 23166 13 21 (ERR-2) Uncertainty due to detector efficiency. 23166 13 22 (MONIT-ERR) Uncertainty of Au c-s. 23166 13 23 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 13 24 (ERR-6) Uncertainty due to time factors . 23166 13 25 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 13 26 (ERR-8) Uncertainty due to time integrated flux. 23166 13 27 (ERR-S) Statistical uncertainty. 23166 13 28 (ERR-T) Total uncertainty 23166 13 29 STATUS (TABLE) Table on p.341 of INDC(GER)-0053 23166 13 30 HISTORY (20211119C) SD 23166 13 31 ENDBIB 29 0 23166 13 32 COMMON 10 6 23166 13 33 KT-DUMMY MONIT MONIT-ERR ERR-1 ERR-2 ERR-5 23166 13 34 ERR-6 ERR-7 ERR-8 ERR-S 23166 13 35 KEV MB PER-CENT PER-CENT PER-CENT PER-CENT 23166 13 36 PER-CENT PER-CENT PER-CENT PER-CENT 23166 13 37 25. 622.7 1.0 0.2 1.5 0.423166 13 38 0.2 0.2 1.5 0.9 23166 13 39 ENDCOMMON 6 0 23166 13 40 DATA 3 4 23166 13 41 DATA ERR-T FLAG 23166 13 42 MB MB NO-DIM 23166 13 43 3.58 0.13 1. 23166 13 44 3.59 0.14 2. 23166 13 45 3.45 0.14 3. 23166 13 46 3.52 0.20 4. 23166 13 47 ENDDATA 6 0 23166 13 48 ENDSUBENT 47 0 23166 1399999 SUBENT 23166014 20211119 230523166 14 1 BIB 7 26 23166 14 2 REACTION 1((30-ZN-68(N,G)30-ZN-69-M,,SIG,,SPA)/ 23166 14 3 (79-AU-197(N,G)79-AU-198,,SIG,,SPA)) 23166 14 4 2(30-ZN-68(N,G)30-ZN-69-M,,SIG,,SPA) 23166 14 5 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 14 6 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 14 7 ANALYSIS Mean value for four runs. 23166 14 8 Measured quantity at kT=25 keV: cross section ratio 23166 14 9 (68Zn(ng)68Zn-m)/197Au = 0.00563+-0.00015 23166 14 10 Cross section value in Subent 23166.005 is 23166 14 11 renormalized for new gold cross section 23166 14 12 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.005 23166 14 13 Because statistical uncertainties were found to 23166 14 14 be practically negligible after averaging the results 23166 14 15 from repeated activations, the final uncertainties are 23166 14 16 determined by systematic effects. 23166 14 17 (ERR-1) Uncertainty due to self-absorption. 23166 14 18 (ERR-2) Uncertainty due to detector efficiency. 23166 14 19 (ERR-3) Uncertainty of Au nuclei number. 23166 14 20 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 14 21 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 14 22 (ERR-6) Uncertainty due to time factors 23166 14 23 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 14 24 (ERR-8) Uncertainty due to time integrated flux. 23166 14 25 STATUS (TABLE) Table on p.342 of INDC(GER)-0053 23166 14 26 (DEP,23166004) See ANALYSIS. 23166 14 27 HISTORY (20211119C) SD 23166 14 28 ENDBIB 26 0 23166 14 29 COMMON 8 6 23166 14 30 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 14 31 ERR-7 ERR-8 23166 14 32 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 14 33 PER-CENT PER-CENT 23166 14 34 0.2 1.5 0.1 0.06 0.4 0.223166 14 35 0.2 1.5 23166 14 36 ENDCOMMON 6 0 23166 14 37 DATA 5 1 23166 14 38 KT-DUMMY DATA 1ERR-T 1DATA 2ERR-T 2 23166 14 39 KEV NO-DIM NO-DIM MB MB 23166 14 40 25. 0.00563 0.00015 3.50 0.09 23166 14 41 ENDDATA 3 0 23166 14 42 ENDSUBENT 41 0 23166 1499999 SUBENT 23166015 20211119 230523166 15 1 BIB 13 36 23166 15 2 REACTION (30-ZN-70(N,G)30-ZN-71-M,,SIG,,SPA) 23166 15 3 DECAY-DATA (30-ZN-71-M,3.96HR,DG,487.30,0.612) 23166 15 4 HL 3.96+-0.05 h, Egamma 487.30 +- 0.04 keV, 23166 15 5 intensity 61.2 +- 2.3%, from REL-REF of K.Abusaleem. 23166 15 6 See also ADD-RES for HL measured in this experiment. 23166 15 7 INC-SPECT Quasistellar neutron spectrum of kT=25 keV. 23166 15 8 MONITOR (79-AU-197(N,G)79-AU-198-G,,SIG,,SPA) 23166 15 9 DECAY-MON (79-AU-198-G,3881.0MIN,DG,411.80,0.9558) 23166 15 10 MONIT-REF (,R.Reifarth+,J,EPJ/P,133,424,2018) 23166 15 11 ANALYSIS Cross section value in Subent 23166.006 is 23166 15 12 renormalized for new gold cross section 23166 15 13 Measured quantity at kT=25 keV: cross section ratio 23166 15 14 (70Zn(ng)71Zn-m)/197Au = 0.01164+-0.00072 23166 15 15 ADD-RES (DECAY) New value of Zn-71-m HL was measured in this 23166 15 16 work from the decay curves of three (386, 487, 620 keV)23166 15 17 gamma transitions in 71Ga to be 4.125 +-0.007 h. 23166 15 18 Combining this new result with the values of previous 23166 15 19 measurements, weighted average of 4.120+-0.007 h was 23166 15 20 obtained 23166 15 21 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 15 22 FLAG (1.) Run I. 23166 15 23 (2.) Run II. 23166 15 24 (3.) Run III. 23166 15 25 (4.) Run IV. 23166 15 26 See details in METHOD and SAMPLE in Subent 001. 23166 15 27 ERR-ANALYS (ERR-1) Uncertainty due to self-absorption. 23166 15 28 (ERR-2) Uncertainty due to detector efficiency. 23166 15 29 (MONIT-ERR) Uncertainty of Au c-s. 23166 15 30 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 15 31 (ERR-6) Uncertainty due to time factors . 23166 15 32 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 15 33 (ERR-8) Uncertainty due to time integrated flux. 23166 15 34 (ERR-S) Statistical uncertainty. 23166 15 35 (ERR-T) Total uncertainty 23166 15 36 STATUS (TABLE) Table on p.343 of INDC(GER)-0053 23166 15 37 HISTORY (20211119C) SD 23166 15 38 ENDBIB 36 0 23166 15 39 COMMON 10 6 23166 15 40 KT-DUMMY MONIT MONIT-ERR ERR-1 ERR-2 ERR-5 23166 15 41 ERR-6 ERR-7 ERR-8 ERR-S 23166 15 42 KEV MB PER-CENT PER-CENT PER-CENT PER-CENT 23166 15 43 PER-CENT PER-CENT PER-CENT PER-CENT 23166 15 44 25. 622.7 1.0 0.2 1.5 0.923166 15 45 1.3 3.8 2.4 0.8 23166 15 46 ENDCOMMON 6 0 23166 15 47 DATA 3 4 23166 15 48 DATA ERR-T FLAG 23166 15 49 MB MB NO-DIM 23166 15 50 7.10 0.40 1. 23166 15 51 7.92 0.43 2. 23166 15 52 6.79 0.37 3. 23166 15 53 7.17 0.47 4. 23166 15 54 ENDDATA 6 0 23166 15 55 ENDSUBENT 54 0 23166 1599999 SUBENT 23166016 20211119 230523166 16 1 BIB 7 26 23166 16 2 REACTION 1((30-ZN-70(N,G)30-ZN-71-M,,SIG,,SPA)/ 23166 16 3 (79-AU-197(N,G)79-AU-198,,SIG,,SPA)) 23166 16 4 2(30-ZN-70(N,G)30-ZN-71-M,,SIG,,SPA) 23166 16 5 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 16 6 ANALYSIS Mean value for four runs. 23166 16 7 Measured quantity at kT=25 keV: cross section ratio 23166 16 8 70Zn(ng)71Zn-m)/197Au = 0.01159+-0.00058 23166 16 9 Cross section value in Subent 23166.007 is 23166 16 10 renormalized for new gold cross section 23166 16 11 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 16 12 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.006 23166 16 13 Because statistical uncertainties were found to 23166 16 14 be practically negligible after averaging the results 23166 16 15 from repeated activations, the final uncertainties are 23166 16 16 determined by systematic effects. 23166 16 17 (ERR-1) Uncertainty due to self-absorption. 23166 16 18 (ERR-2) Uncertainty due to detector efficiency. 23166 16 19 (ERR-3) Uncertainty of Au nuclei number. 23166 16 20 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 16 21 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 16 22 (ERR-6) Uncertainty due to time factors . 23166 16 23 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 16 24 (ERR-8) Uncertainty due to time integrated flux. 23166 16 25 STATUS (TABLE) Table on p.344 of INDC(GER)-0053 23166 16 26 (DEP,23166006) See ANALYSIS. 23166 16 27 HISTORY (20211119C) SD 23166 16 28 ENDBIB 26 0 23166 16 29 COMMON 8 6 23166 16 30 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 16 31 ERR-7 ERR-8 23166 16 32 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 16 33 PER-CENT PER-CENT 23166 16 34 0.2 1.5 0.1 0.06 0.9 1.323166 16 35 3.8 2.4 23166 16 36 ENDCOMMON 6 0 23166 16 37 DATA 5 1 23166 16 38 KT-DUMMY DATA 1ERR-T 1DATA 2ERR-T 2 23166 16 39 KEV NO-DIM NO-DIM MB MB 23166 16 40 25. 0.01159 0.00058 7.21 0.35 23166 16 41 ENDDATA 3 0 23166 16 42 ENDSUBENT 41 0 23166 1699999 SUBENT 23166017 20211119 230523166 17 1 BIB 11 27 23166 17 2 REACTION 1((30-ZN-70(N,G)30-ZN-71-G,,SIG,,SPA)/ 23166 17 3 (79-AU-197(N,G)79-AU-198,,SIG,,SPA)) 23166 17 4 2(30-ZN-70(N,G)30-ZN-71-G,,SIG,,SPA) 23166 17 5 Only run I 23166 17 6 DECAY-DATA (30-ZN-71-G,2.45MIN,DG,910.3,0.0784) 23166 17 7 HL=2.45+-0.10 min, Egamma=910.3 +-0.1 keV, 23166 17 8 intensity 7.84 +- 0.64 %, from REL-REF of K.Abusaleem 23166 17 9 INC-SPECT Quasistellar neutron spectrum of kT-25 keV. 23166 17 10 MONITOR (79-AU-197(N,G)79-AU-198-G,,SIG,,SPA) 23166 17 11 DECAY-MON (79-AU-198-G,3881.0MIN,DG,411.80,0.9558) 23166 17 12 MONIT-REF (,R.Reifarth+,J,EPJ/P,133,424,2018) 23166 17 13 ANALYSIS Cross section value in Subent 23166.008 is 23166 17 14 renormalized for new gold cross section 23166 17 15 Measured quantity at kT=25 keV: cross section ratio 23166 17 16 (70Zn(ng)71Zn-g)/197Au = 0.00713+-0.00011 23166 17 17 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 17 18 ERR-ANALYS (ERR-1) Uncertainty due to self-absorption. 23166 17 19 (ERR-2) Uncertainty due to detector efficiency. 23166 17 20 (MONIT-ERR) Uncertainty of Au c-s. 23166 17 21 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 17 22 (ERR-6) Uncertainty due to time factors . 23166 17 23 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 17 24 (ERR-8) Uncertainty due to time integrated flux. 23166 17 25 (ERR-S) Statistical uncertainty. 23166 17 26 (ERR-T) Total uncertainty 23166 17 27 STATUS (TABLE) Table on p.345 of INDC(GER)-0053 23166 17 28 HISTORY (20211119C) SD 23166 17 29 ENDBIB 27 0 23166 17 30 COMMON 9 6 23166 17 31 MONIT MONIT-ERR ERR-1 ERR-2 ERR-5 ERR-6 23166 17 32 ERR-7 ERR-8 ERR-S 23166 17 33 MB PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 17 34 PER-CENT PER-CENT PER-CENT 23166 17 35 622.7 1.0 0.2 1.5 0.9 4.023166 17 36 8.2 2.5 13. 23166 17 37 ENDCOMMON 6 0 23166 17 38 DATA 5 1 23166 17 39 KT-DUMMY DATA 1ERR-T 1DATA 2ERR-T 2 23166 17 40 KEV NO-DIM NO-DIM MB MB 23166 17 41 25. 0.00713 0.00011 4.44 0.71 23166 17 42 ENDDATA 3 0 23166 17 43 ENDSUBENT 42 0 23166 1799999 SUBENT 23166018 20211119 230523166 18 1 BIB 8 36 23166 18 2 REACTION (30-ZN-64(N,G)30-ZN-65,,SIG,,MXW,DERIV) 23166 18 3 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 18 4 ADD-RES Normalization to the present results for kT = 25 keV 23166 18 5 was done, using data of Z.Y.Bao+: 23166 18 6 KT,keV MACS,mb 23166 18 7 5. 123. 23166 18 8 10. 95.9 23166 18 9 15. 78.2 23166 18 10 20. 66.6 23166 18 11 25. 58.6 +- 1.7 23166 18 12 30. 52.4 +- 1.7 23166 18 13 40. 46.2 23166 18 14 50. 41.7 23166 18 15 60. 39.1 23166 18 16 80. 35.5 23166 18 17 100. 33.7 23166 18 18 REL-REF (R,,Z.Y.Bao+,J,AND,76,70,2000) 23166 18 19 ANALYSIS Data were derived from measure c-s - see CORRECTION. 23166 18 20 Cross section value in Subent 23166.009 is 23166 18 21 renormalized for new gold cross section 23166 18 22 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.009 23166 18 23 Because statistical uncertainties were found to 23166 18 24 be practically negligible after averaging the results 23166 18 25 from repeated activations, the final uncertainties are 23166 18 26 determined by systematic effects. 23166 18 27 (ERR-1) Uncertainty due to self-absorption. 23166 18 28 (ERR-2) Uncertainty due to detector efficiency. 23166 18 29 (ERR-3) Uncertainty of Au nuclei number. 23166 18 30 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 18 31 (ERR-5) Uncertainty due to number of Zn-64 nuclei. 23166 18 32 (ERR-6) Uncertainty due to time factors 23166 18 33 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 18 34 (ERR-8) Uncertainty due to time integrated flux. 23166 18 35 STATUS (TABLE) Table on p.346 of INDC(GER)-0053 23166 18 36 (DEP,23166003) See ANALYSIS. 23166 18 37 HISTORY (20211119C) SD 23166 18 38 ENDBIB 36 0 23166 18 39 COMMON 8 6 23166 18 40 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 18 41 ERR-7 ERR-8 23166 18 42 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 18 43 PER-CENT PER-CENT 23166 18 44 0.2 1.5 0.1 0.06 0.5 0.123166 18 45 0.2 1.5 23166 18 46 ENDCOMMON 6 0 23166 18 47 DATA 3 1 23166 18 48 KT DATA ERR-T 23166 18 49 KEV MB MB 23166 18 50 25. 62.2 1.7 23166 18 51 ENDDATA 3 0 23166 18 52 ENDSUBENT 51 0 23166 1899999 SUBENT 23166019 20211119 230523166 19 1 BIB 8 36 23166 19 2 REACTION (30-ZN-70(N,G)30-ZN-71,,SIG,,MXW,DERIV) 23166 19 3 ADD-RES Normalization to the present results for kT = 25 keV 23166 19 4 was done, using data of Z.Y.Bao+: 23166 19 5 5. 28.4 23166 19 6 10. 18.9 23166 19 7 15. 14.9 23166 19 8 20. 13.1 23166 19 9 25. 11.7 +- 0.8 23166 19 10 30. 10.7 +- 0.8 23166 19 11 40. 9.3 23166 19 12 50. 8.4 23166 19 13 60. 7.7 23166 19 14 80. 6.8 23166 19 15 100. 6.2 23166 19 16 REL-REF (R,,Z.Y.Bao+,J,AND,76,70,2000) 23166 19 17 ANALYSIS Data were derived from measure c-s - see CORRECTION. 23166 19 18 Cross section value in Subent 23166.010 is 23166 19 19 renormalized for new gold cross section 23166 19 20 CORRECTION Correction for revised gold standard: 622.7/586 =1.06223166 19 21 ERR-ANALYS (ERR-T) Error propagation is given in Subent 23166.010 23166 19 22 Because statistical uncertainties were found to 23166 19 23 be practically negligible after averaging the results 23166 19 24 from repeated activations, the final uncertainties are 23166 19 25 determined by systematic effects. 23166 19 26 (ERR-1) Uncertainty due to self-absorption. 23166 19 27 (ERR-2) Uncertainty due to detector efficiency. 23166 19 28 (ERR-3) Uncertainty of Au nuclei number. 23166 19 29 (ERR-4) Uncertainty of gamma-ray intensity for Au. 23166 19 30 (ERR-5) Uncertainty due to number of Zn nuclei. 23166 19 31 (ERR-6) Uncertainty due to time factors . 23166 19 32 (ERR-7) Uncertainty due to gamma-ray intensity for Zn. 23166 19 33 (ERR-8) Uncertainty due to time integrated flux. 23166 19 34 STATUS (TABLE) Table on p.347 of INDC(GER)-0053 23166 19 35 (DEP,23166007) 23166 19 36 (DEP,23166008) 23166 19 37 HISTORY (20211119C) SD 23166 19 38 ENDBIB 36 0 23166 19 39 COMMON 8 6 23166 19 40 ERR-1 ERR-2 ERR-3 ERR-4 ERR-5 ERR-6 23166 19 41 ERR-7 ERR-8 23166 19 42 PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT PER-CENT 23166 19 43 PER-CENT PER-CENT 23166 19 44 0.2 1.5 0.1 0.06 0.9 1.323166 19 45 3.8 2.4 23166 19 46 ENDCOMMON 6 0 23166 19 47 DATA 3 1 23166 19 48 KT DATA ERR-T 23166 19 49 KEV MB MB 23166 19 50 25. 12.4 0.8 23166 19 51 ENDDATA 3 0 23166 19 52 ENDSUBENT 51 0 23166 1999999 ENDENTRY 19 0 2316699999999