Aberle, O.

Andrzejewski, J.

Audouin, L.

Bacak, M.

Balibrea, J.

Barbagallo, M.

Barros, S.

Battino, U.

Beinrucker, C.

Belloni, F.

Berthoumieux, E.

Bečvář, F.

Billowes, J.

Bosnar, D.

Brugger, M.

Bécares, V.

Caamaño, M.

Calviani, M.

Calviño, F.

Cano-Ott, D.

Cerutti, F.

Chiaveri, E.

Colonna, N.

Cortés, G.

Cortés-Giraldo, M. A.

Cosentino, L.

Damone, L. A.

Deo, K.

Diakaki, M.

Dietz, M.

Domingo-Pardo, C.

Dressler, R.

Dupont, E.

Durán, I.

Fernández-Domínguez, B.

Ferrari, A.

Ferreira, P.

Finocchiaro, P.

Frost, R. J. W.

Furman, V.

García, A. R.

Gawlik, A.

Gheorghe, I.

Glodariu, T.

González-Romero, E.

Gonçalves, I. F.

Goverdovski, A.

Griesmayer, E.

Guerrero, C.

Gunsing, F.

Göbel, K.

Harada, H.

Heftrich, T.

Heinitz, S.

Hernández-Prieto, A.

Heyse, J.

Jenkins, D. G.

Jericha, E.

Kadi, Y.

Katabuchi, T.

Kavrigin, P.

Ketlerov, V.

Khryachkov, V.

Kimura, A.

Kivel, N.

Knapova, I.

Kokkoris, M.

Krtička, M.

Käppeler, F.

Leal-Cidoncha, E.

Lederer-Woods, C.

Leeb, H.

Lerendegui-Marco, J.

Licata, M.

Lo Meo, S.

Losito, R.

Macina, D.

Marganiec, J.

Martínez, T.

Massimi, C.

Mastinu, P.

Mastromarco, M.

Matteucci, F.

Mendoza, E.

Mengoni, A.

Milazzo, P. M.

Mingrone, F.

Mirea, M.

Montesano, S.

Musumarra, A.

Nolte, R.

Palomo-Pinto, F. R.

Paradela, C.

Patronis, N.

Pavlik, A.

Perkowski, J.

Porras, J. I.

Praena, J.

Quesada, J. M.

Rauscher, T.

English

Reifarth, R.

Tattersall, A.

Valenta, S.

Weiss, C.

KITopen

Physics Letters B 840 (2023) 137835Contents lists available at ScienceDirectPhysics Letters Bjournal homepage: www.elsevier.com/locate/physletbCorrigendumCorrigendum: “Measurement of 73Ge(n, γ ) cross sections and implications for stellar nucleosynthesis” [Phys. Lett. B 790 (2019) 458–465]C. Lederer-Woods a,b,∗, U. Battino a, P. Ferreira c, A. Gawlik d, C. Guerrero e, F. Gunsing f,g, S. Heinitz h, J. Lerendegui-Marco e, A. Mengoni i, R. Reifarth b, A. Tattersall a, S. Valenta j, C. Weiss g,m, O. Aberle g, J. Andrzejewski d, L. Audouin k, V. Bécares l, M. Bacak m, J. Balibrea l, M. Barbagallo n, S. Barros c, F. Bečvář j, C. Beinrucker b, F. Belloni f, E. Berthoumieux f, J. Billowes o, D. Bosnar p, M. Brugger g, M. Caamaño q, F. Calviño r, M. Calviani g, D. Cano-Ott l, F. Cerutti g, E. Chiaveri g, N. Colonna n, G. Cortés r, M.A. Cortés-Giraldo e, L. Cosentino s, L.A. Damone n,t, K. Deo u, M. Diakaki f,v, M. Dietz a, C. Domingo-Pardo w, R. Dressler h, E. Dupont f, I. Durán q, B. Fernández-Domínguez q, A. Ferrari g, P. Finocchiaro s, R.J.W. Frost o, V. Furman x, K. Göbel b, A.R. García l, I. Gheorghe y, T. Glodariu y, I.F. Gonçalves c, E. González-Romero l, A. Goverdovski z, E. Griesmayer m, H. Harada aa, T. Heftrich b, A. Hernández-Prieto g,r, J. Heyse ab, D.G. Jenkins ac, E. Jericha m, F. Käppeler ad, Y. Kadi g, T. Katabuchi ae, P. Kavrigin m, V. Ketlerov z, V. Khryachkov z, A. Kimura aa, N. Kivel h, I. Knapova j, M. Kokkoris v, M. Krtička j, E. Leal-Cidoncha q, H. Leeb m, M. Licata af,ag, S. Lo Meo i,af, R. Losito g, D. Macina g, J. Marganiec d, T. Martínez l, C. Massimi af,ag, P. Mastinu ah, M. Mastromarco n, F. Matteucci ai,aj, E. Mendoza l, P.M. Milazzo ai, F. Mingrone af, M. Mirea y, S. Montesano g, A. Musumarra s,ak, R. Nolte al, F.R. Palomo-Pinto e, C. Paradela q, N. Patronis am, A. Pavlik an, J. Perkowski d, J.I. Porras g,ao, J. Praena e, J.M. Quesada e, T. Rauscher ap,aq, A. Riego-Perez r, M. Robles q, C. Rubbia g, J.A. Ryan o, M. Sabaté-Gilarte g,e, A. Saxena u, P. Schillebeeckx ab, S. Schmidt b, D. Schumann h, P. Sedyshev x, A.G. Smith o, A. Stamatopoulos v, S.V. Suryanarayana u, G. Tagliente n, J.L. Tain w, A. Tarifeño-Saldivia w, L. Tassan-Got k, A. Tsinganis v, G. Vannini af,ag, V. Variale n, P. Vaz c, A. Ventura af, V. Vlachoudis g, R. Vlastou v, A. Wallner ar, S. Warren o, M. Weigand b, T. Wright o, P. Žugec pa School of Physics and Astronomy, University of Edinburgh, United Kingdomb Goethe University Frankfurt, Germanyc Instituto Superior Técnico, Lisbon, Portugald University of Lodz, Polande Universidad de Sevilla, Spainf CEA Irfu, Université Paris-Saclay, F-91191 Gif-sur-Yvette, Franceg European Organization for Nuclear Research (CERN), Switzerlandh Paul Scherrer Institut (PSI), Villingen, Switzerlandi Agenzia nazionale per le nuove tecnologie, l’energia e lo sviluppo economico sostenibile (ENEA), Bologna, Italyj Charles University, Prague, Czech Republick Institut de Physique Nucléaire, CNRS-IN2P3, Univ. Paris-Sud, Université Paris-Saclay, F-91406 Orsay Cedex, Francel Centro de Investigaciones Energéticas Medioambientales y Tecnológicas (CIEMAT), Spainm Technische Universität Wien, Austrian Istituto Nazionale di Fisica Nucleare, Sezione di Bari, Italyo University of Manchester, United KingdomDOI of original article: https://doi.org/10.1016/j.physletb.2019.01.045.* Corresponding author at: School of Physics and Astronomy, University of Edinburgh, United Kingdom.E-mail address: claudia.lederer-woods@ed.ac.uk (C. Lederer-Woods).https://doi.org/10.1016/j.physletb.2023.1378350370-2693/© 2023 The Author(s). Published by Elsevier B.V. All rights reserved.C. Lederer-Woods, U. Battino, P. Ferreira et al. Physics Letters B 840 (2023) 137835p Department of Physics, Faculty of Science, University of Zagreb, Zagreb, Croatiaq University of Santiago de Compostela, Spainr Universitat Politècnica de Catalunya, Spains INFN Laboratori Nazionali del Sud, Catania, Italyt Dipartimento di Fisica, Università degli Studi di Bari, Italyu Bhabha Atomic Research Centre (BARC), Indiav National Technical University of Athens, Greecew Instituto de Física Corpuscular, CSIC - Universidad de Valencia, Spainx Joint Institute for Nuclear Research (JINR), Dubna, Russiay Horia Hulubei National Institute of Physics and Nuclear Engineering, Romaniaz Institute of Physics and Power Engineering (IPPE), Obninsk, Russiaaa Japan Atomic Energy Agency (JAEA), Tokai-mura, Japanab European Commission, Joint Research Centre, Geel, Retieseweg 111, B-2440 Geel, Belgiumac University of York, United Kingdomad Karlsruhe Institute of Technology, Campus North, IKP, 76021 Karlsruhe, Germanyae Tokyo Institute of Technology, Japanaf Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Italyag Dipartimento di Fisica e Astronomia, Università di Bologna, Italyah Istituto Nazionale di Fisica Nucleare, Sezione di Legnaro, Italyai Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Italyaj Dipartimento di Astronomia, Università di Trieste, Italyak Dipartimento di Fisica e Astronomia, Università di Catania, Italyal Physikalisch-Technische Bundesanstalt (PTB), Bundesallee 100, 38116 Braunschweig, Germanyam University of Ioannina, Greecean University of Vienna, Faculty of Physics, Vienna, Austriaao University of Granada, Spainap Centre for Astrophysics Research, University of Hertfordshire, United Kingdomaq Department of Physics, University of Basel, Switzerlandar Australian National University, Canberra, Australiaa r t i c l e i n f oArticle history:Received 13 February 2023Accepted 6 March 2023Available online 14 March 2023Editor: D.F. GeesamanThe neutron fluence spectrum used in the analysis to deter-mine absolute cross section values was found to be erroneous. The same error also affects data in [1], and a separate correc-tion will be published for that work. The corrected Maxwellian Table 1Ground state Maxwellian averaged cross sections on 73Ge, and stellar Maxwellian averaged cross sections, taking into account neutron capture on thermally populated excited states.kT (keV) MACS (mb) MACS∗ (mb)5 1181 ± 48 1185 ± 5910 722 ± 34 728 ± 5520 455 ± 24 455 ± 4630 346 ± 19 339 ± 3940 284 ± 16 273 ± 3450 243 ± 14 231 ± 3060 214 ± 13 201 ± 2770 192 ± 11 179 ± 2580 175 ± 11 162 ± 2390 161.0 ± 9.7 148 ± 22100 149.7 ± 9.1 137 ± 21Table 2Uncertainties of Maxwellian averaged 73Ge cross sections.Source Uncertainty (%)Neutron Flux Shape 2 − 5Weighting Functions 3Normalisation to Au 1Background Subtraction (> 14 keV) 1Sample Enrichment 1Multiple Scattering andSelf Shielding (> 14 keV) 1.2Statistics 0.3Total 4.1-6.12averaged cross sections (MACS) are listed in Table 1 and shown in Fig. 1. The corrected resonance capture kernels and unresolved cross sections are shown in Tables 3–7, and Fig. 2, respectively. The average resonance parameters determined from the resonance fits change slightly (within uncertainties). We obtain an average radiative width of 〈γ 〉 = 243(10) meV and σγ = 30(5) meV, an average s-wave spacing of D0 = 74(8) eV, and neutron strength functions of S0 = 2.1(3) × 10−4 and S1 = 1.5(5) × 10−4. Uncer-tainties in the resonance kernels due to systematic effects are 3.9% below and 6.0% above 10 keV neutron energy, consisting of uncertainties due to Pulse Height Weighting (3%), normalisa-Fig. 1. Comparison of the experimental MACS from kT = 5 − 100 keV with eval-uations and theoretical predictions [2–8]. MOST-2005 [3] and TALYS-1.9 [4] most closely reproduce the experimental values, while all others significantly underesti-mate the MACS by a factor of up to 2.C. Lederer-Woods, U. Battino, P. Ferreira et al.Fig. 2. Averaged cross sections from 14 keV to 300 keV neutron energy and statisti-cal uncertainties.Table 3Resonance energies and capture kernels k of 73Ge(n, γ ) aResonances fitted with nat-ural germanium sample. ∗Resonances listed in ENDF/B-VIII [2]. b Doublet in ENDF/B-VIII [2].E R (eV) K (meV) E R (eV) K (meV)59.37 ± 0.06 0.0027 ± 0.0005 1219.96 ± 0.02∗ 112.59 ± 0.8979.47 ± 0.01 0.054 ± 0.002 1233.08 ± 0.06 11.05 ± 0.53102.73 ± 0.01a,∗ 104.04 ± 0.63 1276.90 ± 0.05 3.86 ± 0.13156.32 ± 0.02 0.064 ± 0.003 1316.75 ± 0.02∗ 108.65 ± 0.84204.15 ± 0.01a,∗ 60.80 ± 0.51 1358.03 ± 0.02∗ 70.90 ± 0.71224.81 ± 0.00∗ 74.29 ± 0.18 1380.22 ± 0.18 0.91 ± 0.09270.90 ± 0.06 0.073 ± 0.006 1384.69 ± 0.09 1.87 ± 0.11286.68 ± 0.02 0.204 ± 0.007 1404.78 ± 0.09 1.47 ± 0.09320.69 ± 0.01a,∗ 63.83 ± 1.12 1462.39 ± 0.08 3.14 ± 0.15332.87 ± 0.02a,∗ 97.14 ± 1.59 1530.64 ± 0.03∗ 119.8 ± 1.0361.81 ± 0.06 0.47 ± 0.04 1540.43 ± 0.09 3.59 ± 0.22368.07 ± 0.01∗ 95.95 ± 0.32 1549.35 ± 0.13 3.75 ± 0.31409.28 ± 0.00∗ 59.61 ± 0.20 1552.27 ± 0.09 6.28 ± 0.37479.57 ± 0.07 0.56 ± 0.04 1614.59 ± 0.26 0.47 ± 0.07491.48 ± 0.01∗ 101.45 ± 0.47 1655.93 ± 0.05∗ 124.1 ± 1.3517.99 ± 0.01∗ 11.91 ± 0.10 1665.37 ± 0.09 6.19 ± 0.37558.35 ± 0.01∗ 74.05 ± 0.27 1675.03 ± 0.42 0.61 ± 0.12668.80 ± 0.04∗ 0.94 ± 0.03 1716.18 ± 0.04 19.05 ± 0.38693.58 ± 0.04 0.81 ± 0.03 1751.88 ± 0.18 0.98 ± 0.09750.31 ± 0.08 0.31 ± 0.02 1808.03 ± 0.04∗ 111.3 ± 1.1762.71 ± 0.02 3.40 ± 0.06 1843.00 ± 0.08 3.93 ± 0.19777.47 ± 0.04 0.91 ± 0.03 1897.71 ± 0.18 1.15 ± 0.10798.47 ± 0.06 0.44 ± 0.03 1930.82 ± 0.73 0.30 ± 0.09816.68 ± 0.24 0.084 ± 0.015 1952.76 ± 0.05b,∗ 106.6 ± 1.2826.23 ± 0.02 5.04 ± 0.09 1963.42 ± 0.15 3.20 ± 0.27843.31 ± 0.03 2.95 ± 0.09 2019.34 ± 0.05∗ 118.6 ± 1.5851.38 ± 0.01∗ 57.97 ± 0.45 2104.01 ± 0.11 3.43 ± 0.20878.76 ± 0.08 0.73 ± 0.05 2116.60 ± 0.13 3.64 ± 0.21920.47 ± 0.01∗ 48.99 ± 0.46 2144.12 ± 0.17 2.38 ± 0.18948.06 ± 0.13 0.34 ± 0.04 2162.03 ± 0.03 51.86 ± 0.95959.19 ± 0.05 1.72 ± 0.07 2211.39 ± 0.58 0.49 ± 0.111031.14 ± 0.01∗ 56.42 ± 0.65 2216.97 ± 0.51 0.53 ± 0.101059.02 ± 0.01 75.26 ± 0.64 2236.71 ± 0.41 1.03 ± 0.171139.18 ± 0.13 1.82 ± 0.15 2262.52 ± 0.05∗ 109.3 ± 1.61148.41 ± 0.03∗ 119.64 ± 0.86 2291.07 ± 0.13 118.1 ± 4.1tion (1%), sample enrichment (1%), and neutron flux (2% below, 5% above 10 keV). Total systematic uncertainties for the averaged cross sections are 6.2% and uncertainties for the Maxwellian aver-aged capture cross sections change correspondingly (see Table 2). Due to the small changes of at most 4% in the Maxwellian aver-aged capture cross section (smaller than the total uncertainty), all conclusions remain unaltered. The authors apologise for any incon-venience this caused. Updated data will be provided to the EXFOR database.3Physics Letters B 840 (2023) 137835Table 4Table 3 continued.E R (eV) K (meV) E R (eV) K (meV)2297.88 ± 0.07∗ 104.7 ± 3.9 3431.09 ± 0.66 6.8 ± 2.52321.90 ± 0.07 16.70 ± 0.57 3432.30 ± 0.59 7.2 ± 2.52373.27 ± 0.12 6.58 ± 0.34 3495.69 ± 0.54 1.59 ± 0.262398.90 ± 0.29 1.47 ± 0.19 3535.63 ± 0.08 38.8 ± 1.12442.65 ± 0.04 106.7 ± 1.5 3565.09 ± 0.35 3.87 ± 0.422531.55 ± 0.23 2.33 ± 0.22 3579.46 ± 0.08 34.7 ± 1.12566.67 ± 0.06∗ 118.0 ± 1.6 3628.37 ± 0.32 3.49 ± 0.362624.55 ± 0.13 6.96 ± 0.43 3657.50 ± 0.16 17.67 ± 0.872648.06 ± 0.06∗ 26.81 ± 0.69 3674.49 ± 0.06 92.5 ± 2.02666.79 ± 0.05 54.1 ± 1.3 3718.10 ± 0.07 71.0 ± 1.82688.08 ± 0.05 107.2 ± 1.8 3745.17 ± 0.19 9.00 ± 0.542697.88 ± 0.13 8.48 ± 0.53 3763.27 ± 0.25 4.74 ± 0.402748.80 ± 0.39∗ 2.14 ± 0.29 3809.15 ± 0.59 4.15 ± 0.972763.66 ± 0.28 2.79 ± 0.31 3812.80 ± 0.46 3.94 ± 0.852776.01 ± 0.05 48.9 ± 1.0 3852.86 ± 0.15 21.10 ± 0.932806.78 ± 0.18 3.91 ± 0.30 3870.01 ± 0.09 48.3 ± 1.42821.47 ± 0.35 2.05 ± 0.22 3993.95 ± 0.30 7.63 ± 0.672903.85 ± 0.17 5.19 ± 0.35 4002.59 ± 0.44 3.79 ± 0.462924.79 ± 0.14 11.86 ± 0.63 4042.61 ± 0.26 19.1 ± 1.82946.15 ± 0.08 113.0 ± 1.9 4053.75 ± 0.25 143.5 ± 3.92982.64 ± 0.05 52.9 ± 1.2 4073.85 ± 0.08 86.7 ± 3.03005.30 ± 0.86∗ 1.02 ± 0.29 4215.87 ± 0.20 16.47 ± 0.913023.48 ± 0.05 102.0 ± 1.9 4246.62 ± 0.25 107.1 ± 4.13037.63 ± 0.08 36.8 ± 1.2 4254.80 ± 0.12 68.2 ± 3.63044.65 ± 0.61 1.87 ± 0.40 4349.24 ± 0.10∗ 60.3 ± 1.73085.74 ± 0.36 2.25 ± 0.27 4394.73 ± 0.21 16.2 ± 1.03133.34 ± 0.56 1.66 ± 0.29 4406.67 ± 0.14 34.8 ± 1.63155.23 ± 0.06 90.3 ± 1.6 4419.24 ± 0.56∗ 3.80 ± 0.583214.08 ± 0.14 8.93 ± 0.52 4458.64 ± 0.13 134.6 ± 3.03251.24 ± 0.07 29.21 ± 0.84 4475.90 ± 0.29 15.2 ± 1.23264.48 ± 0.43 1.17 ± 0.20 4499.19 ± 0.11 107.0 ± 2.73320.64 ± 0.17 8.74 ± 0.52 4548.87 ± 0.26 16.4 ± 1.23361.67 ± 0.10 38.2 ± 1.2 4564.62 ± 0.10 115.9 ± 2.83388.25 ± 0.29 5.98 ± 0.49 4635.78 ± 0.10 68.9 ± 2.03414.95 ± 0.07 47.6 ± 6.1 4649.66 ± 0.48 4.14 ± 0.58Table 5Table 3 continued.E R (eV) K (meV) E R (eV) K (meV)4753.84 ± 0.46 8.4 ± 1.1 6040.11 ± 0.15 134.7 ± 4.04759.61 ± 0.46 7.5 ± 1.1 6075.57 ± 0.16∗ 120.9 ± 3.94828.05 ± 0.30 29.8 ± 2.1 6136.59 ± 0.60 9.28 ± 0.934837.18 ± 0.35 52.6 ± 5.8 6155.00 ± 0.60 8.6 ± 1.14843.11 ± 0.17 138.2 ± 6.9 6219.66 ± 0.16 149.6 ± 4.44898.05 ± 0.55 6.92 ± 0.81 6241.34 ± 0.16 84.9 ± 3.14949.77 ± 0.29 12.81 ± 0.97 6279.24 ± 0.41 23.2 ± 2.05039.55 ± 0.22 22.3 ± 1.2 6289.64 ± 0.39 23.3 ± 2.15061.31 ± 0.13 57.9 ± 2.2 6327.12 ± 0.41 27.8 ± 2.45098.09 ± 0.41 12.9 ± 1.2 6344.30 ± 0.19 126.8 ± 4.15106.75 ± 0.22∗ 23.4 ± 1.5 6400.4 ± 1.3 4.5 ± 1.35126.36 ± 0.44 6.22 ± 0.74 6427.66 ± 0.19∗ 57.5 ± 2.45160.93 ± 0.41 7.02 ± 0.71 6455.7 ± 1.8 2.95 ± 0.895207.89 ± 0.17 120.5 ± 3.5 6470.55 ± 0.27 38.5 ± 2.35220.23 ± 0.31 2.5 ± 1.2 6485.65 ± 0.38 23.4 ± 1.95245.99 ± 0.14 51.8 ± 1.9 6504.19 ± 0.18 59.2 ± 2.45281.73 ± 0.13 124.4 ± 3.2 6578.24 ± 0.25 134.3 ± 4.95302.89 ± 0.93 6.1 ± 1.2 6602.48 ± 0.36 97 ± 105312.61 ± 0.23 32.3 ± 2.1 6616.73 ± 0.62 160 ± 285364.06 ± 0.24 110.6 ± 4.8 6626.32 ± 0.63 113 ± 215381.64 ± 0.25∗ 132.4 ± 5.4 6739.99 ± 0.26 3.1 ± 1.55419.93 ± 0.12 130.0 ± 3.4 6766.28 ± 0.16 159.5 ± 4.95485.82 ± 0.25 18.3 ± 1.2 6826.23 ± 0.85 8.6 ± 1.25506.04 ± 0.38 9.40 ± 0.85 6866.12 ± 0.21 104.7 ± 3.95547.04 ± 0.45 8.34 ± 0.90 6883.41 ± 0.57 15.8 ± 2.05598.25 ± 0.14∗ 95.6 ± 3.1 6955.69 ± 0.19 91.1 ± 3.45612.69 ± 0.42∗ 8.4 ± 1.0 6974.01 ± 0.59 11.5 ± 1.55681.92 ± 0.37 14.9 ± 1.2 7118.06 ± 0.20∗ 81.2 ± 3.25716.42 ± 0.14 117.9 ± 3.2 7154.31 ± 0.08 12.3 ± 4.45765.08 ± 0.22 138.4 ± 4.2 7177.27 ± 0.38 41.2 ± 2.75815.34 ± 0.22 43.8 ± 2.4 7221.40 ± 0.18 124.4 ± 4.95873.41 ± 0.18 93.4 ± 3.3 7245.55 ± 0.52 24.3 ± 2.45927.51 ± 0.44 9.5 ± 1.6 7290.68 ± 0.27 137.3 ± 5.05975.45 ± 0.64 6.85 ± 0.86 7330.82 ± 0.31 137.2 ± 5.36002.51 ± 0.27 36.4 ± 2.0 7370.58 ± 0.24 90.5 ± 4.0C. Lederer-Woods, U. Battino, P. Ferreira et al. Physics Letters B 840 (2023) 137835Table 6Table 3 continued.E R (eV) K (meV) E R (eV) K (meV)7480.93 ± 0.20 68.5 ± 3.0 9038.39 ± 0.25 129.3 ± 3.37507.9 ± 1.3 7.6 ± 1.5 9086.31 ± 0.54 46.7 ± 4.17601.57 ± 0.22 87.6 ± 3.4 9097.10 ± 0.93 21.6 ± 3.47641.77 ± 0.21 143.1 ± 4.8 9147.3 ± 1.7 15.2 ± 2.77756.09 ± 0.75 15.3 ± 1.8 9168.5 ± 1.3 12.1 ± 2.37777.38 ± 0.35 36.2 ± 2.5 9191.3 ± 1.0 26.2 ± 3.67830.12 ± 0.71 23.5 ± 2.5 9209.90 ± 0.97 51.5 ± 9.97862.18 ± 0.52 114.8 ± 6.1 9222.55 ± 0.57 224 ± 157898.11 ± 0.22 151.4 ± 6.3 9266.86 ± 0.60 44.1 ± 4.17931.39 ± 0.29 63.1 ± 3.5 9319.02 ± 0.47 253.4 ± 9.87971.43 ± 0.33 142.7 ± 5.3 9344.00 ± 0.33 110.7 ± 6.98020.56 ± 0.28 86.2 ± 4.5 9362.65 ± 0.37 16.5 ± 6.48036.77 ± 0.51 30.3 ± 2.8 9490.33 ± 0.26 159.2 ± 5.58099.76 ± 0.26 177.7 ± 5.6 9545.6 ± 1.2 15.0 ± 2.98148.00 ± 0.46 39.1 ± 2.9 9559.01 ± 0.98 22.6 ± 3.38180.99 ± 0.29 89.2 ± 4.4 9575.31 ± 0.81 26.0 ± 3.38328.93 ± 0.35 42.6 ± 2.7 9626.55 ± 0.30 115.2 ± 5.08350.40 ± 0.14 6.8 ± 3.2 9707.4 ± 1.9 10.2 ± 2.78410.58 ± 0.12∗ 3.1 ± 1.5 9728.34 ± 0.37 101.6 ± 5.48441.8 ± 1.0 12.7 ± 2.3 9802.71 ± 0.87 107.0 ± 9.68489.2 ± 2.1 84 ± 15 9816.44 ± 0.48 94.0 ± 8.68507.6 ± 1.0 52 ± 13 9863.39 ± 0.74 22.1 ± 2.78543.20 ± 0.55 23.4 ± 2.5 9966.2 ± 1.1 28.6 ± 4.38589.1 ± 1.0 110.4 ± 7.2 9994.25 ± 0.67 75.9 ± 7.98609.42 ± 0.19 26 ± 10 10009.73 ± 0.48 156 ± 118642.78 ± 0.19 6.2 ± 2.9 10036.7 ± 1.6 25.6 ± 7.08675.04 ± 0.29 80.4 ± 4.1 10044.41 ± 0.68 52.6 ± 7.18713.62 ± 0.33 106.1 ± 5.1 10154.42 ± 0.44 96.6 ± 5.28765.55 ± 0.42 41.3 ± 3.0 10208.14 ± 0.39 149.8 ± 6.48810.90 ± 0.37 65.4 ± 3.9 10356.44 ± 0.43 92.5 ± 4.78833.80 ± 0.60 18.0 ± 1.9 10414.95 ± 0.65 77.0 ± 6.48863.81 ± 0.84 15.6 ± 2.1 10443.80 ± 0.39 199.4 ± 9.38905.6 ± 1.1 9.7 ± 1.6 10475.0 ± 1.3 13.6 ± 2.58921.7 ± 1.2 10.7 ± 1.7 10511.4 ± 1.4 9.0 ± 2.29000.01 ± 0.30∗ 84.7 ± 4.4 10580.2 ± 1.3 36.0 ± 6.3Table 7Table 3 continued.E R (eV) K (meV) E R (eV) K (meV)10598.1 ± 1.0 123 ± 16 11967.31 ± 0.51 153.4 ± 8.610613.34 ± 0.58 103 ± 12 12030.65 ± 0.91 28.0 ± 2.810683.44 ± 0.60 75.1 ± 5.5 12100.51 ± 0.60 106.3 ± 6.210704.73 ± 0.10 13.7 ± 6.3 12180.5 ± 1.1 32.1 ± 3.310745.98 ± 0.70 92.8 ± 9.6 12280.5 ± 1.1 66.8 ± 6.210767.5 ± 1.8 51 ± 17 12323.77 ± 0.65 62.8 ± 5.310776.2 ± 1.3 197 ± 28 12444.2 ± 1.0 45.3 ± 4.810801.26 ± 0.96 35.3 ± 5.8 12558.99 ± 0.63 101.9 ± 7.010851.40 ± 0.41 128.5 ± 7.3 12586.57 ± 0.88 65.2 ± 6.210889.87 ± 0.47 152.3 ± 7.6 12664.81 ± 0.41 133.5 ± 7.510945.21 ± 0.69 27.7 ± 2.6 12757.70 ± 0.58 153.6 ± 8.811085.59 ± 0.84 34.4 ± 3.8 12849.78 ± 0.55 215.8 ± 9.611136.20 ± 0.79 69.3 ± 8.6 12908.7 ± 1.1 32.2 ± 3.711155.5 ± 1.6 139 ± 49 12979.02 ± 0.96 46 ± 611163.3 ± 1.8 150 ± 52 13010.1 ± 1.9 84 ± 1811211.67 ± 0.47 103.6 ± 6.8 13029.0 ± 1.5 101 ± 1811240.47 ± 1.06 18.8 ± 2.8 13071.52 ± 0.15 49 ± 1811317.24 ± 1.95 63.6 ± 8.8 13113.1 ± 1.3 27.0 ± 3.511343.58 ± 0.89 54.5 ± 7.4 13233.98 ± 0.55 144.6 ± 7.411359.97 ± 0.63 59.8 ± 5.7 13289.15 ± 0.59 74.5 ± 5.811409.6 ± 1.0 37.7 ± 4.4 13350.2 ± 1.6 29.3 ± 4.011441.92 ± 0.49 91.6 ± 5.6 13384.1 ± 1.3 51.9 ± 6.311482.5 ± 1.6 15.5 ± 3.1 13407.4 ± 1.6 50.1 ± 8.011525.81 ± 0.14 15.2 ± 6.1 13425.19 ± 0.78 125 ± 1111542.41 ± 0.46 15.1 ± 6.3 13514.8 ± 1.3 84.1 ± 9.511570.32 ± 0.72 70.7 ± 5.8 13551.26 ± 0.54 282 ± 1411597.56 ± 0.98 36.9 ± 4.0 13654.62 ± 0.76 60.2 ± 5.411618.37 ± 0.93 30.2 ± 3.6 13700.12 ± 0.68 103.0 ± 7.011675.01 ± 0.68 107.6 ± 8.6 13740.6 ± 1.4 26.9 ± 3.811700.45 ± 0.64 116.7 ± 9.1 13767.3 ± 1.5 32.3 ± 4.811795.03 ± 0.64 106.6 ± 6.6 13796.7 ± 1.0 49.3 ± 5.211821.0 ± 1.4 18.3 ± 3.1 13857.67 ± 0.75 131 ± 1011856.0 ± 1.6 19.5 ± 3.2 13900.4 ± 1.4 124 ± 1211883.8 ± 1.5 31.5 ± 5.1 13940.8 ± 1.1 87 ± 1011911.03 ± 0.45 170.6 ± 9.2 13967.45 ± 0.75 138 ± 11Data availabilityData will be available in IAEA EXFOR database.AcknowledgementsThis work was supported by the Austrian Science Fund FWF (J3503), the Adolf Messer Foundation (Germany), the UK Science and Technology Facilities Council (ST/M006085/1), and the Euro-pean Research Council ERC-2015-StG Nr. 677497. We acknowledge also support from MSMT of the Czech Republic.References[1] A. Gawlik, et al., Phys. Rev. C 100 (2019) 045804.[2] D.A. Brown, et al., Nucl. Data Sheets 148 (2018) 1–142.[3] S. Goriely, Hauser-Feshbach rates for neutron capture reactions (version 8/29/2005), http://www-astro .ulb .ac .be /Html /hfr.html.[4] A.J. Koning, et al., TALYS-1.9, online at www.talys .eu.[5] A.J. Koning, et al., Nucl. Data Sheets 113 (2012) 2841, https://tendl .web .psi .ch /tendl _2015 /tendl2015 .html.[6] K. Shibata, et al., J. Nucl. Sci. Technol. 48 (2011) 1.[7] JEFF-3.2, available online: http://www.oecd -nea .org /dbforms /data /eva /evatapes /jeff _32/, 2014.[8] I. Dillmann, R. Plag, F. Käppeler, T. Rauscher, EFNUDAT Fast Neutrons - scientific workshop on neutron measurements, theory & applications, JRC-IRMM, 2009;online at http://www.kadonis .org.4

Corrigendum: “Measurement of ⁷³Ge(n,γ) cross sections and implications for stellar nucleosynthesis” [Phys. Lett. B 790 (2019) 458–465]

https://publikationen.bibliothek.kit.edu/1000157267/150518218

Corrigendum: “Measurement of ⁷³Ge(n,γ) cross sections and implications for stellar nucleosynthesis” [Phys. Lett. B 790 (2019) 458–465]

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