ENTRY C1487 20230802 C231C1487000 1 SUBENT C1487001 20230802 C231C1487001 1 BIB 11 33 C1487001 2 INSTITUTE (1USAANL,3ISLHEB,1USANWU) C1487001 3 REFERENCE (J,PR/C,67,065809,2003) C1487001 4 #doi:10.1103/PhysRevC.67.065809 C1487001 5 AUTHOR (K.E.Rehm,A.H.Wuosmaa,C.L.Jiang,J.Caggiano,J.P.Greene, C1487001 6 A.Heinz,D.Henderson,R.V.F.Janssens,E.F.Moore, C1487001 7 G.Mukherjee,R.C.Pardo,T.Pennington,J.P.Schiffer, C1487001 8 R.H.Siemssen) C1487001 9 TITLE Branching ratio Galpha/Ggamma of the 4.033 MeV 3/2+ C1487001 10 state in 19Ne C1487001 11 FACILITY (CYCLO,1USAANL) C1487001 12 INC-SPECT The 20Ne beam bombarded a 1.5-mm-long gas cell filled C1487001 13 with 3He at 700 mbar. C1487001 14 SAMPLE The gas target was cooled to liquid nitrogen C1487001 15 temperature, resulting in a 3He thickness of 50 C1487001 16 microg/cm2. The pressure in the 3He target was kept C1487001 17 constant to better than 1%. C1487001 18 DETECTOR (SIBAR) The outgoing a particles from the C1487001 19 3He(20Ne,a)19Ne reaction were detected in a Si strip C1487001 20 detector telescope consisting of a 500-mm-thick, 40x40C1487001 21 mm2 DE detector backed by a 50x50 mm2, 300-mm-thick C1487001 22 Eres detector tilted by an angle of 50 degree in orderC1487001 23 to increase its effective thickness for the incident C1487001 24 particles to about 500 mm. The DE detector was C1487001 25 subdivided in the front and back into 32 vertical and C1487001 26 horizontal strips (1-mm width) which were read out C1487001 27 individually. C1487001 28 METHOD Inverse kinematics C1487001 29 (EDE) C1487001 30 MONITOR The telescope was calibrated using a 228Th a source andC1487001 31 energy resolutions of 45 keV for the DE and Eres C1487001 32 detectors were obtained. C1487001 33 HISTORY (20061217C) DR C1487001 34 (20230726A) OS. REACTION correction in sub.2 C1487001 35 ENDBIB 33 0 C1487001 36 NOCOMMON 0 0 C1487001 37 ENDSUBENT 36 0 C148700199999 SUBENT C1487002 20230802 C231C1487002 1 BIB 4 9 C1487002 2 REACTION 1(8-O-15(A,0),,EN) C1487002 3 2(8-O-15(A,G),,WID) C1487002 4 3(8-O-15(A,0),,J) C1487002 5 4(8-O-15(A,0),,PTY) C1487002 6 ERR-ANALYS2(+DATA-ERR) Total superior uncertainty C1487002 7 (-DATA-ERR) Total inferior uncertainty C1487002 8 STATUS (TABLE,,K.E.Rehm+,J,PR/C,67,065809,2003) Table 2 C1487002 9 HISTORY (20230726A) SF3 corrected in REACTION 4; ERR-T changed C1487002 10 to DATA-ERR C1487002 11 ENDBIB 9 0 C1487002 12 NOCOMMON 0 0 C1487002 13 DATA 6 6 C1487002 14 DATA 1DATA 2+DATA-ERR 2-DATA-ERR 2DATA 3DATA 4C1487002 15 MEV MILLI-EV MILLI-EV MILLI-EV NO-DIM NO-DIM C1487002 16 0.504 12. 9. 5. 1.5 +1. C1487002 17 0.850 458. 92. 92. 4.5 -1. C1487002 18 1.020 39. 34. 1.5 1.5 -1. C1487002 19 1.071 101. 55. 55. 2.5 +1. C1487002 20 1.183 43. 8. 8. 2.5 -1. C1487002 21 1.563 196. 39. 39. 2.5 +1. C1487002 22 ENDDATA 8 0 C1487002 23 ENDSUBENT 22 0 C148700299999 SUBENT C1487003 20061218 C079C148700300001 BIB 4 7 C148700300002 REACTION 1(8-O-15(A,0),,EN) C148700300003 2(8-O-15(A,G),,WID/STR) C148700300004 ERR-ANALYS (+ERR-T) Total superior uncertainty C148700300005 (-ERR-T) Total inferior uncertainty C148700300006 FLAG (1.) Calculated assuming spectroscopic factors of 0.1 C148700300007 for the alpha width. C148700300008 STATUS (TABLE) Data taken from Table 2 C148700300009 ENDBIB 7 0 C148700300010 NOCOMMON 0 0 C148700300011 DATA 5 8 C148700300012 DATA 1DATA 2+ERR-T 2-ERR-T 2FLAG C148700300013 MEV MILLI-EV MILLI-EV MILLI-EV NO-DIM C148700300014 0.504 2.5E-02 C148700300015 0.611 5.7E-04 1. C148700300016 0.668 8.9E-03 1. C148700300017 0.850 2.9E+01 11. 11. C148700300018 1.020 4.E+00 3.5 1.5 C148700300019 1.071 9.0E+01 50. 50. C148700300020 1.183 1.10E+02 21. 21. C148700300021 1.563 5.30E+02 110. 110. C148700300022 ENDDATA 10 0 C148700300023 ENDSUBENT 22 0 C148700399999 ENDENTRY 3 0 C148799999999