ENTRY C2454 20201020 C202C245400000001 SUBENT C2454001 20201020 C202C245400100001 BIB 10 35 C245400100002 TITLE Gamma-ray spectroscopy of astrophysically important C245400100003 states in 39Ca C245400100004 AUTHOR (M.R.Hall,D.W.Bardayan,T.Baugher,A.Lepailleur,S.D.Pain,C245400100005 A.Ratkiewicz,S.Ahn,J.M.Allen,J.T.Anderson, C245400100006 A.D.Ayangeakaa,J.C.Blackmon,S.Burcher,M.P.Carpenter, C245400100007 S.M.Cha,K.Y.Chae,K.A.Chipps,J.A.Cizewski,M.Febbraro, C245400100008 O.Hall,J.Hu,C.L.Jiang,K.L.Jones,E.J.Lee,P.D.O'Malley, C245400100009 S.Ota,B.C.Rasco,D.Santiago-Gonzalez,D.Seweryniak, C245400100010 H.Sims,K.Smith,W.P.Tan,P.Thompson,C.Thornsberry, C245400100011 R.L.Varner,D.Walter,G.L.Wilson,S.Zhu) C245400100012 INSTITUTE (1USANOT,1USAORL,1USARUT,1USAMSU,1USAANL,1USALSU, C245400100013 1USACLI,2UK SUR,1USALRL,1USALTI,1USABNL) C245400100014 (3KORKOR) Sungkyunkwan University, Suwon C245400100015 REFERENCE (J,PR/C,101,015804,2020) C245400100016 FACILITY (LINAC,1USAANL) Experiment performed at the ATLAS C245400100017 accelerator at Argonne National Laboratory C245400100018 SAMPLE CaF2 target with thickness of 938 mu-g/cm2 C245400100019 DETECTOR The gamma rays and reaction alpha particles were C245400100020 measured in coincidence using Gammasphere ORRUBA Dual C245400100021 Detectors for Experimental Structure Studies GODDESS. C245400100022 GODDESS combines HPGe detector array Gammasphere C245400100023 and charged particle barrel array ORRUBA. C245400100024 (HPGE) Gamma rays were detected using Gammasphere C245400100025 array of 110 HPGe detectors covering almost 4Pi solid C245400100026 angle around the target. C245400100027 (TELES,SISD,SISD) Charged particles were measured C245400100028 using six de-E telsecopes. Each telescope consisted C245400100029 of 65 mu-m thick dE deteector and 1000 mu-m thick E C245400100030 detector. ORRUBA covered angular angle of C245400100031 approximatelly 45deg-90deg. C245400100032 METHOD (COINC) Coincidence between gamma rays and charged C245400100033 particles was required. C245400100034 CORRECTION Gamma spectra from Gammasphere were corrected for C245400100035 Doppler effect. C245400100036 HISTORY (20201020C) Compiled by S.H. C245400100037 ENDBIB 35 0 C245400100038 NOCOMMON 0 0 C245400100039 ENDSUBENT 38 0 C245400199999 SUBENT C2454002 20201020 C202C245400200001 BIB 3 3 C245400200002 REACTION (19-K-38(P,G),,WID/STR) C245400200003 ERR-ANALYS (DATA-ERR) Origin of uncertainties not described C245400200004 STATUS (TABLE) Data taken from tab. 2 of the reference C245400200005 ENDBIB 3 0 C245400200006 NOCOMMON 0 0 C245400200007 DATA 6 3 C245400200008 EN-RES EN-RES-ERR DATA DATA-ERR DATA-MIN DATA-MAX C245400200009 KEV KEV MILLI-EV MILLI-EV MILLI-EV MILLI-EV C245400200010 386. 2. 2.54 C245400200011 498. 2. 2.47 24.7 C245400200012 701. 2. 126. 39. C245400200013 ENDDATA 5 0 C245400200014 ENDSUBENT 13 0 C245400299999 ENDENTRY 2 0 C245499999999