ENTRY C2771 20241030 C247C277100000001 SUBENT C2771001 20241030 C247C277100100001 BIB 10 23 C277100100002 TITLE Revised decay properties of the key 93-keV resonance C277100100003 in the 25Mg(p,gamma) reaction and its influence on C277100100004 the MgAl cycle in astrophysical environments C277100100005 AUTHOR (G.Lotay,D.T.Doherty,R.V.F.Janssens,D.Seweryniak, C277100100006 H.M.Albers,S.Almaraz-Calderon,M.P.Carpenter, C277100100007 A.E.Champagne,C.J.Chiara,C.R.Hoffman,C.Iliadis, C277100100008 A.Kankainen,T.Lauritsen,S.Zhu) C277100100009 REFERENCE (J,PR/C,105,L042801,2022) C277100100010 #doi:10.1103/PhysRevC.105.L042801 C277100100011 REL-REF (O,C2595002,A.Kankainen+,J,PL/B,813,136033,2021) C277100100012 INSTITUTE (2UK SUR,1USANCA,1USATNL,1USAANL,1USAMRY,2SF JYV) C277100100013 FACILITY (LINAC,1USAANL) The Argonne ATLAS accelerator. C277100100014 DETECTOR (HPGE) The Gammasphere detector array which, in this C277100100015 instance, consisted of 99 detectors operated in C277100100016 stand-alone mode. C277100100017 SAMPLE ~300 mu-g/cm2-thick target of 11B. C277100100018 METHOD ~5 pnA, 19-MeV beam of 16O ions, delivered by the C277100100019 Argonne ATLAS accelerator, was used to bombard 11B C277100100020 target for ~100 hr, in order to populate excited C277100100021 states in 26Al via the one-neutron evaporation C277100100022 channel. The resulting gamma-ray transitions were C277100100023 detected using the Gammasphere array. C277100100024 HISTORY (20241030C) BP C277100100025 ENDBIB 23 0 C277100100026 COMMON 1 3 C277100100027 EN C277100100028 MEV C277100100029 19. C277100100030 ENDCOMMON 3 0 C277100100031 ENDSUBENT 30 0 C277100199999 SUBENT C2771002 20241030 C247C277100200001 BIB 4 8 C277100200002 REACTION (5-B-11(8-O-16,N)13-AL-26,PAR,DA,G,LEG/RS) C277100200003 ANALYSIS For strong transitions, an angular distribution C277100200004 analysis was performed by fitting gamma-ray intensitiesC277100200005 as a function of detection angle with respect to the C277100200006 beam axis with the customary function C277100200007 W(theta) = A0 [1 + a2P2(cos theta) + a4P4(cos theta)]. C277100200008 ERR-ANALYS (DATA-ERR) No details on sources of uncertainties. C277100200009 STATUS (TABLE,,G.Lotay+,J,PR/C,105,L042801,2022) Table I. C277100200010 ENDBIB 8 0 C277100200011 NOCOMMON 0 0 C277100200012 DATA 4 26 C277100200013 E NUMBER DATA DATA-ERR C277100200014 KEV NO-DIM NO-DIM NO-DIM C277100200015 1744. 2. -0.34 0.06 C277100200016 1744. 4. 0.08 0.08 C277100200017 1894. 2. -0.36 0.11 C277100200018 1894. 4. 0.21 0.14 C277100200019 3239. 2. 0.34 0.15 C277100200020 3239. 4. -0.03 0.17 C277100200021 3999. 2. 0.32 0.11 C277100200022 3999. 4. 0.20 0.14 C277100200023 4130. 2. 0.22 0.06 C277100200024 4130. 4. -0.16 0.09 C277100200025 4273. 2. -0.49 0.08 C277100200026 4273. 4. 0.05 0.08 C277100200027 4328. 2. 0.50 0.11 C277100200028 4328. 4. -0.04 0.14 C277100200029 4749. 2. 0.13 0.20 C277100200030 4749. 4. 0.38 0.24 C277100200031 4806. 2. 0.39 0.07 C277100200032 4806. 4. 0.11 0.11 C277100200033 4851. 2. -0.49 0.16 C277100200034 4851. 4. -0.05 0.21 C277100200035 5743. 2. 0.34 0.08 C277100200036 5743. 4. -0.07 0.10 C277100200037 6018. 2. 0.29 0.06 C277100200038 6018. 4. -0.33 0.09 C277100200039 6193. 2. 0.18 0.04 C277100200040 6193. 4. 0.10 0.05 C277100200041 ENDDATA 28 0 C277100200042 ENDSUBENT 41 0 C277100299999 ENDENTRY 2 0 C277199999999