ENTRY O2520 20210318 O084O252000000001 SUBENT O2520001 20210318 O084O252000100001 BIB 8 32 O252000100002 TITLE Direct measurements of low-energy resonance strengths O252000100003 of the 23Na(p,gamma)24Mg reaction for astrophysics O252000100004 AUTHOR (A.Boeltzig, A.Best, F.R.Pantaleo, G.Imbriani, O252000100005 M.Junker, M.Aliotta, J.Balibrea-Correa, D.Bemmerer, O252000100006 C.Broggini, C.G.Bruno, R.Buompane, A.Caciolli, O252000100007 F.Cavanna, T.Chillery, G.F.Ciani, P.Corvisiero, O252000100008 L.Csedreki, T.Davinson, R.J.Deboer, R.Depalo, O252000100009 A.Di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, O252000100010 A.Formicola, Zs.Fueloep, G.Gervino, A.Guglielmetti, O252000100011 C.Gustavino, Gy.Gyuerky, I.Kochanek, M.Lugaro, O252000100012 P.Marigo, R.Menegazzo, V.Mossa, F.Munnik, V.Paticchio,O252000100013 R.Perrino, D.Piatti, P.Prati, L.Schiavulli, O252000100014 K.Stoeckel, O.Straniero, F.Strieder, T.Szuecs, O252000100015 M.P.Takacs, D.Trezzi, M.Wiescher, S.Zavatarelli) O252000100016 INSTITUTE (2ITYLGS,1USANOT,2ITYNAP,2ITYBAU,2UK EDG,2GERZFK, O252000100017 2ITYFSN,2ITYUPV,2ITYGVA,3HUNDEB,2ITYTUR,2ITYMIL, O252000100018 2GERDRE,2ITYOAC) O252000100019 (2ITYITY) Istituto Nazionale di Fisica Nucleare, O252000100020 Sezione di Roma, P00185 Roma, Italy O252000100021 (3HUNHUN) Konkoly Observatory, Research Centre for O252000100022 Astronomy and Earth Sciences, Hungarian Academy of O252000100023 Sciences, 1121 Budapest, Hungary O252000100024 (1USAUSA) South Dakota School of Mines and Technology, O252000100025 Rapid City, USA O252000100026 REFERENCE (J,PL/B,795,122,2019) O252000100027 #doi:10.1016/j.physletb.2019.05.044 O252000100028 FACILITY (CCW,2ITYLGS) LUNA accelerator. O252000100029 SAMPLE Na2WO4 compound with a thickness of 50 ug/cm2 onto a O252000100030 high purity tantalum backing. The effective stopping O252000100031 power on the order of 10%. O252000100032 METHOD (BCINT,GSPEC) O252000100033 HISTORY (20210318C) VS O252000100034 ENDBIB 32 0 O252000100035 NOCOMMON 0 0 O252000100036 ENDSUBENT 35 0 O252000199999 SUBENT O2520002 20210318 O084O252000200001 BIB 4 10 O252000200002 REACTION 1(11-NA-23(P,0),,EN) O252000200003 2(11-NA-23(P,G),,WID/STR) O252000200004 DETECTOR (HPGE) O252000200005 ERR-ANALYS (ERR-T) All uncertainties are given at 68% CL O252000200006 (ERR-1) uncertainty of the effective stopping power O252000200007 of the material at the resonance energy is the was O252000200008 the dominant contribution to the resonance strength O252000200009 uncertainty - 15% O252000200010 (ERR-2) uncertainty of the accumulated charge - 3% O252000200011 STATUS (TABLE) Table 3 of Phys.Lett.B795(2019)122 O252000200012 ENDBIB 10 0 O252000200013 COMMON 2 3 O252000200014 ERR-1 ERR-2 O252000200015 PER-CENT PER-CENT O252000200016 15. 3. O252000200017 ENDCOMMON 3 0 O252000200018 DATA 3 2 O252000200019 DATA 1DATA 2ERR-T 2 O252000200020 KEV EV EV O252000200021 251. 4.82E-4 8.4E-5 O252000200022 309. 1.08E-1 1.9E-2 O252000200023 ENDDATA 4 0 O252000200024 ENDSUBENT 23 0 O252000299999 SUBENT O2520003 20210319 O084O252000300001 BIB 5 13 O252000300002 REACTION 1(11-NA-23(P,0),,EN) O252000300003 2(11-NA-23(P,G),,WID/STR) O252000300004 DETECTOR (BGO) O252000300005 ANALYSIS The 309 keV resonance was used as a reference O252000300006 to account for the influence of target composition O252000300007 variations on the yield. O252000300008 (UNFLD) The beam-induced backgrounds from O252000300009 7Li(p,gamma)8Be and 11B(p,gamma)12C in the sum energy O252000300010 spectrum were taken into account by a Bayesian approachO252000300011 using Poisson-likelihood for the bin contents. O252000300012 ERR-ANALYS (DATA-ERR) The shortest interval to contain 68% O252000300013 probability ranges from 0.94 and 2.05 meV. O252000300014 STATUS (TABLE) Table 3 of Phys.Lett.B795(2019)122 O252000300015 ENDBIB 13 0 O252000300016 NOCOMMON 0 0 O252000300017 DATA 4 1 O252000300018 DATA 1DATA 2-DATA-ERR 2+DATA-ERR 2 O252000300019 KEV EV EV EV O252000300020 140. 1.46E-9 5.3E-10 5.8E-10 O252000300021 ENDDATA 3 0 O252000300022 ENDSUBENT 21 0 O252000399999 ENDENTRY 3 0 O252099999999