ENTRY C1487 20061218 C079C148700000001 SUBENT C1487001 20061218 C079C148700100001 BIB 11 31 C148700100002 INSTITUTE (1USAANL,3ISLHEB,1USANWU) C148700100003 REFERENCE (J,PR/C,67,065809,2003) C148700100004 AUTHOR (K.E.Rehm,A.H.Wuosmaa,C.L.Jiang,J.Caggiano,J.P.Greene, C148700100005 A.Heinz,D.Henderson,R.V.F.Janssens,E.F.Moore, C148700100006 G.Mukherjee,R.C.Pardo,T.Pennington,J.P.Schiffer, C148700100007 R.H.Siemssen) C148700100008 TITLE Branching ratio Galpha/Ggamma of the 4.033 MeV 3/2+ C148700100009 state in 19Ne C148700100010 FACILITY (CYCLO,1USAANL) C148700100011 INC-SPECT The 20Ne beam bombarded a 1.5-mm-long gas cell filled C148700100012 with 3He at 700 mbar. C148700100013 SAMPLE The gas target was cooled to liquid nitrogen C148700100014 temperature, resulting in a 3He thickness of 50 C148700100015 microg/cm2. The pressure in the 3He target was kept C148700100016 constant to better than 1%. C148700100017 DETECTOR (SIBAR) The outgoing a particles from the C148700100018 3He(20Ne,a)19Ne reaction were detected in a Si strip C148700100019 detector telescope consisting of a 500-mm-thick, 40x40C148700100020 mm2 DE detector backed by a 50x50 mm2, 300-mm-thick C148700100021 Eres detector tilted by an angle of 50 degree in orderC148700100022 to increase its effective thickness for the incident C148700100023 particles to about 500 mm. The DE detector was C148700100024 subdivided in the front and back into 32 vertical and C148700100025 horizontal strips (1-mm width) which were read out C148700100026 individually. C148700100027 METHOD Inverse kinematics C148700100028 (EDE) C148700100029 MONITOR The telescope was calibrated using a 228Th a source andC148700100030 energy resolutions of 45 keV for the DE and Eres C148700100031 detectors were obtained. C148700100032 HISTORY (20061217C) DR C148700100033 ENDBIB 31 0 C148700100034 NOCOMMON 0 0 C148700100035 ENDSUBENT 34 0 C148700199999 SUBENT C1487002 20061218 C079C148700200001 BIB 3 7 C148700200002 REACTION 1(8-O-15(A,0),,EN) C148700200003 2(8-O-15(A,G),,WID) C148700200004 3(8-O-15(A,0),,J) C148700200005 4(8-O-15(A,G),,PTY) C148700200006 ERR-ANALYS (+ERR-T) Total superior uncertainty C148700200007 (-ERR-T) Total inferior uncertainty C148700200008 STATUS (TABLE) Data taken from Table 2 C148700200009 ENDBIB 7 0 C148700200010 NOCOMMON 0 0 C148700200011 DATA 6 6 C148700200012 DATA 1DATA 2+ERR-T 2-ERR-T 2DATA 3DATA 4C148700200013 MEV MILLI-EV MILLI-EV MILLI-EV NO-DIM NO-DIM C148700200014 0.504 12. 9. 5. 1.5 +1. C148700200015 0.850 458. 92. 92. 4.5 -1. C148700200016 1.020 39. 34. 1.5 1.5 -1. C148700200017 1.071 101. 55. 55. 2.5 +1. C148700200018 1.183 43. 8. 8. 2.5 -1. C148700200019 1.563 196. 39. 39. 2.5 +1. C148700200020 ENDDATA 8 0 C148700200021 ENDSUBENT 20 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