ENTRY C2594 20210318 C202C259400000001 SUBENT C2594001 20210318 C202C259400100001 BIB 11 35 C259400100002 TITLE Exploiting Isospin Symmetry to Study the Role of C259400100003 Isomers in Stellar Environments C259400100004 AUTHOR (S.Hallam,G.Lotay,A.Gade,D.T.Doherty,J.Belarge, C259400100005 P.C.Bender,B.A.Brown,J.Browne,W.N.Catford,B.Elman, C259400100006 A.Estrade,M.R.Hall,B.Longfellow,E.Lunderberg,F.Montes, C259400100007 M.Moukaddam,P.O'Malley,W.-J.Ong,H.Schatz,D.Seweryniak, C259400100008 K.Schmidt,N.K.Timofeyuk,D.Weisshaar,R.G.T.Zegers) C259400100009 INSTITUTE (2UK SUR,1USAMSU,1USANOT,1USAANL) C259400100010 (1USAUSA) Central Michigan University, Mount Pleasant C259400100011 REFERENCE (J,PRL,126,042701,2021) C259400100012 FACILITY (CYCTM,1USAMSU) Experiment performed at the cyclotron C259400100013 facility at the National Superconducting Cyclotron C259400100014 Laboratory,Argonne C259400100015 SAMPLE Deuterated polyethylene (CD2)n target with thickness C259400100016 of (9.1+-0.7) mg/cm2. C259400100017 DETECTOR (MAGSP) Projectile-like reaction products were C259400100018 momentum analyzed and transmitted to the focal plane C259400100019 of the S800 spectrometer, which was run in a C259400100020 focused mode and provided clean identification of C259400100021 27Si ions. C259400100022 (HPGE) Prompt gamma rays were detected using GRETINA C259400100023 tracking array. It comprised of 10 modules positioned C259400100024 at laboratory angles of 58 deg and 90 deg. C259400100025 CORRECTION Gamma ray energies were Doppler-corrected. C259400100026 METHOD (TOF,COINC) Coincidence between gamma rays in GRETINA C259400100027 and 27Si recoils in S800 spectrograph was required C259400100028 INC-SOURCE A beam of radioactive 26Si ions was produced by C259400100029 projectile fragmentation of 150 MeV/A primary 36Ar C259400100030 beam. Secondary energy of 26Si ions was 30 MeV/A, C259400100031 beam purity was (60+-5) % and typical intensity C259400100032 approx. 1E+5 ions/s. Time of flight measrements C259400100033 upstream and downstream of the target allowed C259400100034 identification of incomming 26Si ions on event by C259400100035 event basis. C259400100036 HISTORY (20210318C) Compiled by S.H. C259400100037 ENDBIB 35 0 C259400100038 NOCOMMON 0 0 C259400100039 ENDSUBENT 38 0 C259400199999 SUBENT C2594002 20210318 C202C259400200001 BIB 3 4 C259400200002 REACTION ((1-H-2(14-SI-26,P)14-SI-27,PAR,SIG,G)= C259400200003 (14-SI-26(D,P)14-SI-27,PAR,SIG,G)) C259400200004 ERR-ANALYS (DATA-ERR) Origin of uncertainty not described C259400200005 STATUS (TABLE) Data taken from tab.1 of the reference PRL C259400200006 ENDBIB 4 0 C259400200007 COMMON 1 3 C259400200008 EN C259400200009 MEV/A C259400200010 30.0 C259400200011 ENDCOMMON 3 0 C259400200012 DATA 4 12 C259400200013 E LVL-INI DATA DATA-ERR C259400200014 KEV KEV MICRO-B MICRO-B C259400200015 781. 781. 780. 170. C259400200016 957. 957. 610. 140. C259400200017 1690. 2647. 300. 90. C259400200018 2163. 2163. 440. 110. C259400200019 2866. 2866. 1790. 390. C259400200020 3328. 4285. 380. 140. C259400200021 3671. 6319. 2850. 650. C259400200022 4893. 5850. 491. 130. C259400200023 5246. 6027. 170. 80. C259400200024 5629. 6586. 200. 60. C259400200025 5778. 6559. 550. 200. C259400200026 7262. 7262. 160. 60. C259400200027 ENDDATA 14 0 C259400200028 ENDSUBENT 27 0 C259400299999 ENDENTRY 2 0 C259499999999