Publications of Arthur E. Champagne    :recent first  alphabetical  by type listing:

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@article{fds324767,
   Author = {Champagne, AE and Wiescher, M},
   Title = {Explosive hydrogen burning},
   Journal = {Annual Review of Nuclear and Particle Science},
   Volume = {42},
   Number = {1},
   Pages = {39-76},
   Publisher = {ANNUAL REVIEWS},
   Year = {1992},
   Month = {January},
   url = {http://dx.doi.org/10.1146/annurev.ns.42.120192.000351},
   Doi = {10.1146/annurev.ns.42.120192.000351},
   Key = {fds324767}
}

@article{fds324766,
   Author = {Brown, BA and Champagne, AE and Fortune, HT and Sherr,
             R},
   Title = {Nature of the Na20 2646-keV level and the stellar reaction
             rate for Ne19(p,γ)20Na},
   Journal = {Physical Review C},
   Volume = {48},
   Number = {3},
   Pages = {1456-1459},
   Publisher = {American Physical Society (APS)},
   Year = {1993},
   Month = {January},
   url = {http://dx.doi.org/10.1103/PhysRevC.48.1456},
   Abstract = {Careful comparison of F20 and Na20, and available data on
             reactions leading to both, suggests that Jπ(2646)=3+. Other
             mirror identifications are indicated and quantities of
             astrophysical interest are calculated. © 1993 The American
             Physical Society.},
   Doi = {10.1103/PhysRevC.48.1456},
   Key = {fds324766}
}

@article{fds324765,
   Author = {Champagne, AE and Brown, BA and Sherr, R},
   Title = {The 26Al(p, γ)27Si reaction at low stellar
             temperature},
   Journal = {Nuclear Physics A},
   Volume = {556},
   Number = {1},
   Pages = {123-135},
   Publisher = {Elsevier BV},
   Year = {1993},
   Month = {May},
   url = {http://dx.doi.org/10.1016/0375-9474(93)90242-p},
   Doi = {10.1016/0375-9474(93)90242-p},
   Key = {fds324765}
}

@article{fds324763,
   Author = {Mao, ZQ and Vogelaar, RB and Champagne, AE and Blackmon, JC and Das, RK and Hahn, KI and Yuan, J},
   Title = {States in12B and primordial nucleosynthesis.
             (II). Resonance properties and astrophysical
             aspects},
   Journal = {Nuclear Physics A},
   Volume = {567},
   Number = {1},
   Pages = {125-145},
   Publisher = {Elsevier BV},
   Year = {1994},
   Month = {January},
   url = {http://dx.doi.org/10.1016/0375-9474(94)90730-7},
   Abstract = {The9Be(α, p)12B has been used to populate states which
             could correspond to astrophysically significant resonances
             in the8Li(α, n)11B reaction. The branching ratios for
             neutron decays have been measured and the neutron angular
             distributions have been used to determine Jπfor these
             states. This information, combined with previous
             measurements of excitation energies and total widths, allows
             us to extract the resonance strengths for these states. The
             astrophysical significance of these results is discussed. ©
             1994.},
   Doi = {10.1016/0375-9474(94)90730-7},
   Key = {fds324763}
}

@article{fds324764,
   Author = {Mao, ZQ and Vogelaar, RB and Champagne, AE},
   Title = {States in12B and primordial nucleosynthesis. (I).
             Spectroscopic measurements},
   Journal = {Nuclear Physics A},
   Volume = {567},
   Number = {1},
   Pages = {111-124},
   Publisher = {Elsevier BV},
   Year = {1994},
   Month = {January},
   url = {http://dx.doi.org/10.1016/0375-9474(94)90729-3},
   Abstract = {The9Be(α, p)12B and11B(d, p)12B reactions have been used to
             determine excitation energies, total widths and
             spin-parities for states which could correspond to
             astrophysically significant resonances in the8Li(α, n)11B
             reaction. Six such states are observed at Ex= 10.199,
             10.417, 10.564, 10.880, 11.328 and 11.571 MeV. None of these
             states corresponds to the broad resonance observed in
             the11B(n, α)8Li reaction. However, we find no evidence that
             such a resonance exists. © 1994.},
   Doi = {10.1016/0375-9474(94)90729-3},
   Key = {fds324764}
}

@article{fds324762,
   Author = {Hindi, MM and Champagne, AE and da Cruz, MTF and Larimer, R-M and Lesko,
             KT and Norman, EB and Sur, B},
   Title = {β+decay and cosmic-ray half-lives ofPm143andPm144},
   Journal = {Physical Review C},
   Volume = {50},
   Number = {2},
   Pages = {728-732},
   Publisher = {American Physical Society (APS)},
   Year = {1994},
   Month = {August},
   url = {http://dx.doi.org/10.1103/physrevc.50.728},
   Doi = {10.1103/physrevc.50.728},
   Key = {fds324762}
}

@article{fds324761,
   Author = {Blackmon, JC and Champagne, AE and Hofstee, MA and Smith, MS and Downing, RG and Lamaze, GP},
   Title = {Measurement of theO17(p,α)N14Cross Section at Stellar
             Energies},
   Journal = {Physical Review Letters},
   Volume = {74},
   Number = {14},
   Pages = {2642-2645},
   Publisher = {American Physical Society (APS)},
   Year = {1995},
   Month = {April},
   url = {http://dx.doi.org/10.1103/physrevlett.74.2642},
   Doi = {10.1103/physrevlett.74.2642},
   Key = {fds324761}
}

@article{fds324760,
   Author = {Hofstee, MA and Blackmon, JC and Champagne, AE and Bateman, NPT and Parker, PD and Yildiz, K and Young, BM and Vogelaar, RB and Smith, MS and Howard, AJ},
   Title = {Investigating the astrophysically important Ex = 2.646 MeV
             state in 20Na},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             B: Beam Interactions With Materials and Atoms},
   Volume = {99},
   Number = {1-4},
   Pages = {346-348},
   Publisher = {Elsevier BV},
   Year = {1995},
   Month = {May},
   url = {http://dx.doi.org/10.1016/0168-583x(95)00307-x},
   Doi = {10.1016/0168-583x(95)00307-x},
   Key = {fds324760}
}

@article{fds324759,
   Author = {El Eid and MF and Champagne, AE},
   Title = {Sodium enrichment in A-F type supergiants},
   Journal = {The Astrophysical Journal},
   Volume = {451},
   Number = {1},
   Pages = {298-307},
   Publisher = {IOP Publishing},
   Year = {1995},
   Month = {September},
   url = {http://dx.doi.org/10.1086/176219},
   Abstract = {We have investigated the nucleosynthesis of sodium (23Na) in
             stars of masses M = 5-19 M⊙ having solar-like initial
             chemical composition. The values obtained for the Na excess
             after the first dredge-up phase are in close agreement with
             recent observations suggesting a moderate Na excess in
             F-type supergiants. We also found a positive correlation
             between the overabundance factors [N/H] and [Na/H] which
             seems to indicate that Na enrichment originates from the
             Ne-Na cycle operating simultaneously with the CNO tri-cycle
             in these stars. We emphasize that our results were obtained
             on the basis of standard physical assumptions in the stellar
             model calculations, but with updated reaction rates for the
             reactions involved in the Ne-Na cycle which are presented in
             this work.},
   Doi = {10.1086/176219},
   Key = {fds324759}
}

@article{fds324757,
   Author = {Hahn, KI and García, A and Adelberger, EG and Magnus, PV and Bacher,
             AD and Bateman, N and Berg, GPA and Blackmon, JC and Champagne, AE and Davis, B and Howard, AJ and Liu, J and Lund, B and Mao, ZQ and Markoff, DM and Parker, PD and Smith, MS and Stephenson, EJ and Swartz, KB and Utku, S and Vogelaar, RB and Yildiz, K},
   Title = {Structure of 18Ne and the breakout from the hot
             CNO cycle},
   Journal = {Physical Review C},
   Volume = {54},
   Number = {4},
   Pages = {1999-2013},
   Publisher = {American Physical Society (APS)},
   Year = {1996},
   Month = {January},
   url = {http://dx.doi.org/10.1103/PhysRevC.54.1999},
   Abstract = {We used the 16O(3He,n)18Ne, 12C(12C,6He)18Ne, and
             20Ne(p,t)18Ne reactions to study 18Ne states up to an
             excitation energy of 10 MeV, with emphasis on levels
             corresponding to 14O(α,p)17F and 17F(p,γ)18Ne resonances
             that could strongly affect these reaction rates in hot
             stellar environments. Excitation energies, widths, absolute
             cross sections, and angular distributions were measured. We
             found previously unidentified states at Ex=6.15±0.01 MeV,
             7.12±0.02 MeV, 7.35±0.02 MeV, 7.62±0.02 MeV, 8.30±0.02
             MeV, (8.45 ±0.03 MeV), 8.55±0.03 MeV, 8.94±0.02 MeV, and
             9.58±0.02 MeV. We combined level width, cross section, and
             angular distribution data to infer Jπ values for a number
             of the new levels as well as for the previously known
             5.1-MeV doublet. Using information from our experiments, we
             recalculated the 14O(α.p) 17F reaction rate, which
             constitutes a possible path out of the hot CNO cycle into
             the rp process and could play an important role in
             transforming nuclei involved in the hot CNO cycle into
             heavier nuclei with Z≥10.},
   Doi = {10.1103/PhysRevC.54.1999},
   Key = {fds324757}
}

@article{fds324758,
   Author = {Blackmon, JC and Champagne, AE and Dickens, JK and Harvey, JA and Hofstee, MA and Kopecky, S and Larson, DC and Powell, DC and Raman, S and Smith, MS},
   Title = {Measurement of 7Li(n, gamma 0)8Li cross sections at
             En=1.5-1340 eV.},
   Journal = {Physical Review C},
   Volume = {54},
   Number = {1},
   Pages = {383-388},
   Year = {1996},
   Month = {July},
   url = {http://dx.doi.org/10.1103/physrevc.54.383},
   Doi = {10.1103/physrevc.54.383},
   Key = {fds324758}
}

@article{fds324042,
   Author = {Moltz, DM and Powell, JD and Rice, A and Rowe, MW and Cerny, J and Hansper,
             V and Wulf, E and Weller, HR and Champagne, AE and Hofstee,
             M},
   Title = {Measurement of the (7)BE(p,gamma) cross section at low
             energies.},
   Journal = {Abstracts of Papers of the American Chemical
             Society},
   Volume = {213},
   Pages = {43-NUCL},
   Year = {1997},
   Month = {April},
   Key = {fds324042}
}

@article{fds324756,
   Author = {Wallerstein, G and Iben, I and Parker, P and Boesgaard, AM and Hale, GM and Champagne, AE and Barnes, CA and Käppeler, F and Smith, VV and Hoffman,
             RD and Timmes, FX and Sneden, C and Boyd, RN and Meyer, BS and Lambert,
             DL},
   Title = {Synthesis of the elements in stars: Forty years of
             progress},
   Journal = {Reviews of Modern Physics},
   Volume = {69},
   Number = {4},
   Pages = {995-1084},
   Publisher = {American Physical Society (APS)},
   Year = {1997},
   Month = {October},
   url = {http://dx.doi.org/10.1103/revmodphys.69.995},
   Abstract = {Forty years ago Burbidge, Burbidge, Fowler, and Hoyle
             combined what we would now call fragmentary evidence from
             nuclear physics, stellar evolution and the abundances of
             elements and isotopes in the solar system as well as a few
             stars into a synthesis of remarkable ingenuity. Their review
             provided a foundation for forty years of research in all of
             the aspects of low energy nuclear experiments and theory,
             stellar modeling over a wide range of mass and composition,
             and abundance studies of many hundreds of stars, many of
             which have shown distinct evidence of the processes
             suggested by B2FH. In this review we summarize progress in
             each of these fields with emphasis on the most recent
             developments.},
   Doi = {10.1103/revmodphys.69.995},
   Key = {fds324756}
}

@article{fds324755,
   Author = {Wiescher, M and Schatz, H and Champagne, AE},
   Title = {Reactions with radioactive beams and explosive
             nucleosynthesis},
   Journal = {Philosophical Transactions. Series A, Mathematical,
             Physical, and Engineering Sciences},
   Volume = {356},
   Number = {1744},
   Pages = {2105-2136},
   Publisher = {The Royal Society},
   Year = {1998},
   Month = {September},
   url = {http://dx.doi.org/10.1098/rsta.1998.0265},
   Abstract = {This paper summarizes our present understanding of nuclear
             reactions with short-lived particles, which are relevant for
             the nucleosynthesis and energy generation in explosive
             stellar scenarios. It discusses the need for data on
             reactions far off stability and presents a short description
             of the present possibilities for measurements with
             radioactive beams. The paper presents an overview of the
             nucleosynthesis aspects for different explosive burning
             scenarios. The possible influence of proton capture
             reactions on short-lived nuclei are discussed for explosive
             hydrogen burning in novae and X-ray bursts. Also discussed
             are various aspects of weak-interaction processes during the
             collapse phase of a type-II supernova. Finally, we present
             key reactions for the onset of the α recombination in the
             neutrino-driven shock of type-II supernovae, and discuss
             nuclear structure effects for the r-process
             path.},
   Doi = {10.1098/rsta.1998.0265},
   Key = {fds324755}
}

@article{fds324754,
   Author = {Adelberger, EG and Austin, SM and Bahcall, JN and Balantekin, AB and Bogaert, G and Brown, LS and Buchmann, L and Cecil, FE and Champagne,
             AE and de Braeckeleer, L and Duba, CA and Elliott, SR and Freedman, SJ and Gai, M and Goldring, G and Gould, CR and Gruzinov, A and Haxton, WC and Heeger, KM and Henley, E and Johnson, CW and Kamionkowski, M and Kavanagh, RW and Koonin, SE and Kubodera, K and Langanke, K and Motobayashi, T and Pandharipande, V and Parker, P and Robertson, RGH and Rolfs, C and Sawyer, RF and Shaviv, N and Shoppa, TD and Snover, KA and Swanson, E and Tribble, RE and Turck-Chièze, S and Wilkerson,
             JF},
   Title = {Solar fusion cross sections},
   Journal = {Reviews of Modern Physics},
   Volume = {70},
   Number = {4},
   Pages = {1265-1291},
   Publisher = {American Physical Society (APS)},
   Year = {1998},
   Month = {October},
   url = {http://dx.doi.org/10.1103/revmodphys.70.1265},
   Doi = {10.1103/revmodphys.70.1265},
   Key = {fds324754}
}

@article{fds324753,
   Author = {Powell, D and Iliadis, C and Champagne, A and Hale, S and Hansper, V and Surman, R and Veal, K},
   Title = {Low-energy resonance strengths for proton capture on Mg and
             Al nuclei},
   Journal = {Nuclear Physics A},
   Volume = {644},
   Number = {4},
   Pages = {263-276},
   Year = {1998},
   Month = {December},
   url = {http://dx.doi.org/10.1016/S0375-9474(98)00593-4},
   Doi = {10.1016/S0375-9474(98)00593-4},
   Key = {fds324753}
}

@article{fds324752,
   Author = {Powell, DC and Iliadis, C and Champagne, AE and Grossmann, CA and Hale,
             SE and Hansper, VY and McLean, LK},
   Title = {Reaction rate of Mg-24(p,gamma)Al-25},
   Journal = {Nuclear Physics A},
   Volume = {660},
   Number = {3},
   Pages = {349-378},
   Year = {1999},
   Month = {November},
   url = {http://dx.doi.org/10.1016/S0375-9474(99)00390-5},
   Doi = {10.1016/S0375-9474(99)00390-5},
   Key = {fds324752}
}

@article{fds324751,
   Author = {Hansper, VY and Champagne, AE and Hale, SE and Iliadis, C and Powell,
             DC},
   Title = {Measurement of the40Ca(3He,t)40Screaction},
   Journal = {Physical Review C},
   Volume = {61},
   Number = {2},
   Publisher = {American Physical Society (APS)},
   Year = {2000},
   Month = {January},
   url = {http://dx.doi.org/10.1103/physrevc.61.028801},
   Doi = {10.1103/physrevc.61.028801},
   Key = {fds324751}
}

@article{fds324750,
   Author = {Champagne, AE},
   Title = {N-14(p,gamma) O-15 at low stellar temperatures.},
   Journal = {Abstracts of Papers of the American Chemical
             Society},
   Volume = {220},
   Pages = {U10-U10},
   Year = {2000},
   Month = {August},
   Key = {fds324750}
}

@article{fds324749,
   Author = {Mosher, J and Iliadis, C and Bertone, PF and Champagne, AE and Ross, JG and Stephan, A},
   Title = {Nuclear recoil detection with microchannel
             plates},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {459},
   Number = {3},
   Pages = {532-542},
   Publisher = {Elsevier BV},
   Year = {2001},
   Month = {March},
   url = {http://dx.doi.org/10.1016/s0168-9002(00)01056-1},
   Doi = {10.1016/s0168-9002(00)01056-1},
   Key = {fds324749}
}

@article{fds324748,
   Author = {Runkle, RC and Champagne, AE and Engel, J},
   Title = {Thermal Equilibration of26Al},
   Journal = {The Astrophysical Journal},
   Volume = {556},
   Number = {2},
   Pages = {970-978},
   Publisher = {IOP Publishing},
   Year = {2001},
   Month = {August},
   url = {http://dx.doi.org/10.1086/321594},
   Doi = {10.1086/321594},
   Key = {fds324748}
}

@article{fds324747,
   Author = {Bertone, PF and Champagne, AE and Powell, DC and Iliadis, C and Hale,
             SE and Hansper, VY},
   Title = {Lifetime of the 6793-keV state in 15O.},
   Journal = {Physical Review Letters},
   Volume = {87},
   Number = {15},
   Pages = {152501},
   Year = {2001},
   Month = {October},
   url = {http://dx.doi.org/10.1103/physrevlett.87.152501},
   Abstract = {The energy derived from the CN cycle at low stellar
             temperatures is regulated by the 14N(p,gamma)15O reaction. A
             previous direct measurement of this reaction has been
             interpreted as showing evidence for a subthreshold resonance
             which makes a major contribution to the reaction rate at low
             temperatures. This resonance, at E(c.m.) = -504 keV would
             correspond to the known Ex = 6793-keV state in 15O. We have
             measured a mean lifetime of 1.60(+0.75)(-0.72) fs (90% C.L.)
             for this state using the Doppler-shift attenuation method.
             This lifetime is a factor of 15 longer than that inferred
             from the (p,gamma) data and implies that the contribution of
             the subthreshold resonance is negligible.},
   Doi = {10.1103/physrevlett.87.152501},
   Key = {fds324747}
}

@article{fds324746,
   Author = {Hale, S and Champagne, A and Iliadis, C and Hansper, V and Powell, D and Blackmon, J},
   Title = {Investigation of the 22Ne(p,γ)23Na reaction via (3He,d)
             spectroscopy},
   Journal = {Physical Review C},
   Volume = {65},
   Number = {1},
   Publisher = {American Physical Society (APS)},
   Year = {2001},
   Month = {December},
   url = {http://dx.doi.org/10.1103/physrevc.65.015801},
   Doi = {10.1103/physrevc.65.015801},
   Key = {fds324746}
}

@article{fds324743,
   Author = {Caggiano, JA and Bradfield-Smith, W and Lewis, R and Parker, PD and Visser, DW and Greene, JP and Rehm, KE and Bardayan, DW and Champagne,
             AE},
   Title = {Identification of new states in [Formula Presented] using
             the [Formula Presented] reaction and consequences for the
             [Formula Presented] reaction rate in explosive hydrogen
             burning environments},
   Journal = {Physical Review C},
   Volume = {65},
   Number = {5},
   Pages = {6},
   Publisher = {American Physical Society (APS)},
   Year = {2002},
   Month = {January},
   url = {http://dx.doi.org/10.1103/PhysRevC.65.055801},
   Abstract = {We have studied the [Formula Presented] reaction and have
             identified new states in [Formula Presented] at [Formula
             Presented] and [Formula Presented] Based on these
             measurements and other recent evidence, we suggest
             spin-parity assignments of [Formula Presented] for the 5.678
             MeV state and [Formula Presented] for the 5.945 MeV state,
             which would account for all the “missing” unnatural
             parity states in [Formula Presented] in the excitation
             energy region important to hydrogen burning in novae. New
             reaction rates are presented for the [Formula Presented]
             reaction based on this possible assignment of states. ©
             2002 The American Physical Society.},
   Doi = {10.1103/PhysRevC.65.055801},
   Key = {fds324743}
}

@article{fds324745,
   Author = {Rowland, C and Iliadis, C and Champagne, A and Dummer, A and Fitzgerald,
             R and Harley, E and Mosher, J and Runkle, R},
   Title = {Studies of weak capture-γ-ray resonances via coincidence
             techniques},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {480},
   Number = {2-3},
   Pages = {610-625},
   Year = {2002},
   Month = {March},
   url = {http://dx.doi.org/10.1016/S0168-9002(01)01231-1},
   Doi = {10.1016/S0168-9002(01)01231-1},
   Key = {fds324745}
}

@article{fds324744,
   Author = {Rowland, C and Iliadis, C and Champagne, AE and Mosher,
             J},
   Title = {Measurement of theER=338 keVresonance strength
             for23Na(p,α)20Ne},
   Journal = {Physical Review C},
   Volume = {65},
   Number = {6},
   Publisher = {American Physical Society (APS)},
   Year = {2002},
   Month = {May},
   url = {http://dx.doi.org/10.1103/physrevc.65.064609},
   Doi = {10.1103/physrevc.65.064609},
   Key = {fds324744}
}

@article{fds324742,
   Author = {Runkle, RC and Champagne, AE and Fox, C and Iliadis, C and Pollanen, J and Stephan, A and Westerfeldt, C},
   Title = {Search for a resonance in the14N(p,γ)15Oreaction
             atEp=127keV},
   Journal = {Physical Review C},
   Volume = {66},
   Number = {2},
   Publisher = {American Physical Society (APS)},
   Year = {2002},
   Month = {August},
   url = {http://dx.doi.org/10.1103/physrevc.66.022801},
   Doi = {10.1103/physrevc.66.022801},
   Key = {fds324742}
}

@article{fds324741,
   Author = {Bertone, PF and Champagne, AE and Boswell, M and Iliadis, C and Hale,
             SE and Hansper, VY and Powell, DC},
   Title = {14N(3He,d)15Oas a probe of direct capture in
             the14N(p,γ)15Oreaction},
   Journal = {Physical Review C},
   Volume = {66},
   Number = {5},
   Publisher = {American Physical Society (APS)},
   Year = {2002},
   Month = {November},
   url = {http://dx.doi.org/10.1103/physrevc.66.055804},
   Doi = {10.1103/physrevc.66.055804},
   Key = {fds324741}
}

@article{fds324740,
   Author = {Iliadis, C and Champagne, AE and Jose, J and Starrfield, S and Tupper,
             P},
   Title = {Element synthesis in novae},
   Journal = {Revista Mexicana de Física},
   Volume = {49},
   Pages = {45-49},
   Year = {2003},
   Month = {November},
   Key = {fds324740}
}

@article{fds324739,
   Author = {Fox, C and Iliadis, C and Champagne, AE and Coc, A and José, J and Longland, R and Newton, J and Pollanen, J and Runkle,
             R},
   Title = {Explosive hydrogen burning of 17O in classical
             novae.},
   Journal = {Physical Review Letters},
   Volume = {93},
   Number = {8},
   Pages = {081102},
   Year = {2004},
   Month = {August},
   url = {http://dx.doi.org/10.1103/physrevlett.93.081102},
   Abstract = {We report on the observation of a new resonance at
             E(lab)(R)=190 keV in the 17O(p,gamma)18F reaction. The
             measured resonance strength amounts to omegagamma(pgamma)=(1.2+/-0.2)x10(-6)
             eV. With this new value, the uncertainties in the
             17O(p,gamma)18F and 17O(p,alpha)14N thermonuclear reaction
             rates are reduced by orders of magnitude at nova
             temperatures. Our significantly improved reaction rates have
             major implications for the galactic synthesis of 17O, the
             stellar production of the radioisotope 18F, and the
             predicted oxygen isotopic ratios in nova
             ejecta.},
   Doi = {10.1103/physrevlett.93.081102},
   Key = {fds324739}
}

@article{fds324738,
   Author = {Hale, SE and Champagne, AE and Iliadis, C and Hansper, VY and Powell,
             DC and Blackmon, JC},
   Title = {Investigation of theNa23(p,γ)Mg24andNa23(p,α)Ne20reactions
             via(He3,d)spectroscopy},
   Journal = {Physical Review C},
   Volume = {70},
   Number = {4},
   Publisher = {American Physical Society (APS)},
   Year = {2004},
   Month = {October},
   url = {http://dx.doi.org/10.1103/physrevc.70.045802},
   Doi = {10.1103/physrevc.70.045802},
   Key = {fds324738}
}

@article{fds324737,
   Author = {Rowland, C and Iliadis, C and Champagne, AE and Fox, C and José, J and Runkle, R},
   Title = {Does an NeNa Cycle Exist in Explosive Hydrogen
             Burning?},
   Journal = {The Astrophysical Journal},
   Volume = {615},
   Number = {1},
   Pages = {L37-L40},
   Year = {2004},
   Month = {November},
   url = {http://dx.doi.org/10.1086/425964},
   Doi = {10.1086/425964},
   Key = {fds324737}
}

@article{fds324041,
   Author = {Aalseth, CE and Anderson, D and Arthur, R and Avignone, FT and Baktash,
             C and Ball, T and Barabash, AS and Brodzinski, RL and Brudanin, VB and Bugg, W and Champagne, AE and Chan, YD and Cianciolo, TV and Collar, JI and Creswick, RW and Doe, PJ and Dunham, G and Easterday, S and Efremenko,
             YV and Egorov, VG and Ejiri, H and Elliott, SR and Ely, J and Fallon, P and Farach, HA and Gaitskell, RJ and Gehman, V and Grzywacz, R and Hazma, R and Hime, H and Hossbach, T and Jordan, D and Kazkaz, K and Kephart, J and King, GS and Kochetov, OI and Konovalov, SI and Kouzes, RT and Lesko,
             KT and Macchiavelli, AO and Miley, HS and Mills, GB and Nomachi, M and Palms, JM and Pitts, WK and Poon, AWP and Radford, DC and Reeves, JH and Robertson, RGH and Rohm, RM and Rykaczewski, K and Saborov, K and Sandukovsky, VG and Shawley, C and Stekhanov, VN and Tornow, W and Van
             De Water and RG and Vetter, K and Warner, RA and Webb, J and Wilkerson, JF and Wouters, JM and Young, AR and Yumatov, VI},
   Title = {The Majorana neutrinoless double-beta decay
             experiment},
   Journal = {Physics of Atomic Nuclei},
   Volume = {67},
   Number = {11},
   Pages = {2002-2010},
   Publisher = {Pleiades Publishing Ltd},
   Year = {2004},
   Month = {November},
   url = {http://dx.doi.org/10.1134/1.1825519},
   Abstract = {The proposed Majorana double-beta decay experiment is based
             on an array of segmented intrinsic Ge detectors with a total
             mass of 500 kg of Ge isotopically enriched to 86% in 76Ge. A
             discussion is given of background reduction by material
             selection, detector segmentation, pulse shape analysis, and
             electroformation of copper parts and granularity.
             Predictions of the experimental sensitivity are given. For
             an experimental running time of 10 years over the
             construction and operation of the Majorana setup, a
             sensitivity of T1/20ν ∼ 4 × 1027 yr is predicted. This
             corresponds to 〈mν〉 ∼0.003-0.004 eV according to
             recent QRPA and RQRPA matrix element calculations. © 2004
             MAIK "Nauka/Interperiodica".},
   Doi = {10.1134/1.1825519},
   Key = {fds324041}
}

@article{fds324040,
   Author = {Aalseth, CE and Anderson, D and Arthur, R and Avignone, FT and Baktash,
             C and Ball, T and Barabash, AS and Bertrand, F and Brodzinski, RL and Brudanin, V and Bugg, W and Champagne, AE and Chan, YD and Cianciolo,
             TV and Collar, JI and Creswick, RW and Descovich, M and Di Marco and M and Doe, PJ and Dunham, G and Efremenko, Y and Egerov, V and Ejiri, H and Elliott, SR and Emanuel, A and Fallon, P and Farach, HA and Gaitskell,
             RJ and Gehman, V and Grzywacz, R and Hallin, A and Hazma, R and Henning, R and Hime, A and Hossbach, T and Jordan, D and Kazkaz, K and Kephart, J and King, GS and Kochetov, O and Konovalov, S and Kouzes, RT and Lesko, KT and Luke, P and Luzum, M and Macchiavelli, AO and McDonald, A and Mei, D and Miley, HS and Mills, GB and Mokhtarani, A and Nomachi, M and Orrell, JL and Palms, JM and Poon, AWP and Radford, DC and Reeves, JH and Robertson,
             RGH and Runkle, R and Rykaczewski, K and Saburov, K and Sandukovsky, Y and Sonnenschein, A and Tornow, W and Tull, C and van de Water, RG and Vanushin, I and Vetter, K and Warner, RA and Wilkerson, JF and Wouters,
             JM and Young, AR and Yumatov, V},
   Title = {The proposed Majorana 76Ge double-beta decay
             experiment},
   Journal = {Nuclear Physics B Proceedings Supplements},
   Volume = {138},
   Number = {1-3},
   Pages = {217-220},
   Publisher = {Elsevier BV},
   Year = {2005},
   Month = {January},
   url = {http://dx.doi.org/10.1016/j.nuclphysbps.2004.11.052},
   Abstract = {The proposed Majorana experiment is based on an array of
             segmented intrinsic Ge detectors with a total mass of 500 kg
             of Ge isotopically enriched to 86% in 76Ge. Background
             reduction will be accomplished by: material selection,
             detector segmentation, pulse shape analysis,
             electro-formation of copper parts, and granularity of
             detector spacing. The predicted experimental sensitivity for
             measurement of the neutrinoless double-beta decay mode of
             76Ge, over a data acquisition period of 5000 kg·y, is
             T1/20ν ∼ 4×1027y. © 2004 Published by Elsevier
             B.V.},
   Doi = {10.1016/j.nuclphysbps.2004.11.052},
   Key = {fds324040}
}

@article{fds324736,
   Author = {Runkle, RC and Champagne, AE and Angulo, C and Fox, C and Iliadis, C and Longland, R and Pollanen, J},
   Title = {Direct measurement of the 14N(p,gamma)15O S
             factor.},
   Journal = {Physical Review Letters},
   Volume = {94},
   Number = {8},
   Pages = {082503},
   Year = {2005},
   Month = {March},
   url = {http://dx.doi.org/10.1103/physrevlett.94.082503},
   Abstract = {The 14N(p,gamma)15O reaction regulates the rate of energy
             generation in the stellar CN cycle. Because discrepancies
             have been found in the analysis and interpretation of
             previous capture data, we have measured the 14N(p,gamma)15O
             excitation function for energies in the range
             E(lab)(p)=155-524 keV. Fits of these data using R-matrix
             theory yield a value for the S factor at zero energy of
             1.68+/-0.09(stat)+/-0.16(syst) keV b, which is significantly
             smaller than the previous result. The corresponding
             reduction in the stellar reaction rate for 14N(p,gamma)15O
             has a number of interesting consequences, including an
             impact on estimates for the age of the Galaxy derived from
             globular clusters.},
   Doi = {10.1103/physrevlett.94.082503},
   Key = {fds324736}
}

@article{fds324735,
   Author = {Fox, C and Iliadis, C and Champagne, AE and Fitzgerald, RP and Longland,
             R and Newton, J and Pollanen, J and Runkle, R},
   Title = {Thermonuclear reaction rate ofO17(p,γ)F18},
   Journal = {Physical Review C},
   Volume = {71},
   Number = {5},
   Publisher = {American Physical Society (APS)},
   Year = {2005},
   Month = {May},
   url = {http://dx.doi.org/10.1103/physrevc.71.055801},
   Doi = {10.1103/physrevc.71.055801},
   Key = {fds324735}
}

@article{fds324733,
   Author = {Iliadis, C and Champagne, A},
   Title = {Nuclear Astrophysics: Direct measurements with stable
             beams},
   Journal = {Nuclear Physics A},
   Volume = {758},
   Pages = {73-79},
   Year = {2005},
   Month = {July},
   url = {http://dx.doi.org/10.1016/j.nuclphysa.2005.05.019},
   Doi = {10.1016/j.nuclphysa.2005.05.019},
   Key = {fds324733}
}

@article{fds324734,
   Author = {Angulo, C and Champagne, A and Trautvetter, H-P},
   Title = {R-matrix analysis of the 14N(p,γ)15O astrophysical
             S-factor},
   Journal = {Nuclear Physics A},
   Volume = {758},
   Pages = {391-394},
   Year = {2005},
   Month = {July},
   url = {http://dx.doi.org/10.1016/j.nuclphysa.2005.05.070},
   Doi = {10.1016/j.nuclphysa.2005.05.070},
   Key = {fds324734}
}

@article{fds324732,
   Author = {Champagne, AE},
   Title = {Amazing developments in nuclear astrophysics},
   Journal = {The European Physical Journal A},
   Volume = {25},
   Number = {S1},
   Pages = {623-628},
   Year = {2005},
   Month = {September},
   url = {http://dx.doi.org/10.1140/epjad/i2005-06-103-4},
   Doi = {10.1140/epjad/i2005-06-103-4},
   Key = {fds324732}
}

@article{fds324731,
   Author = {Longland, R and Iliadis, C and Champagne, A and Fox, C and Newton,
             J},
   Title = {Nuclear astrophysics studies at the LENA facility: The -ray
             detection system},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {566},
   Number = {2},
   Pages = {452-464},
   Year = {2006},
   Month = {October},
   url = {http://dx.doi.org/10.1016/j.nima.2006.07.006},
   Doi = {10.1016/j.nima.2006.07.006},
   Key = {fds324731}
}

@article{fds324730,
   Author = {CHAMPAGNE, AE and ILIADIS, C},
   Title = {FIRST RESULTS FROM LENA},
   Journal = {Modern Physics Letters A},
   Volume = {22},
   Number = {04},
   Pages = {243-257},
   Publisher = {World Scientific Pub Co Pte Lt},
   Year = {2007},
   Month = {February},
   url = {http://dx.doi.org/10.1142/s0217732307022724},
   Doi = {10.1142/s0217732307022724},
   Key = {fds324730}
}

@article{fds324729,
   Author = {Newton, JR and Iliadis, C and Champagne, AE and Coc, A and Parpottas, Y and Ugalde, C},
   Title = {Gamow peak in thermonuclear reactions at high
             temperatures},
   Journal = {Physical Review C},
   Volume = {75},
   Number = {4},
   Publisher = {American Physical Society (APS)},
   Year = {2007},
   Month = {April},
   url = {http://dx.doi.org/10.1103/physrevc.75.045801},
   Doi = {10.1103/physrevc.75.045801},
   Key = {fds324729}
}

@article{fds324728,
   Author = {Newton, JR and Iliadis, C and Champagne, AE and Longland, R and Ugalde,
             C},
   Title = {Remeasurement of the 193 keV resonance inO17(p,α)N14},
   Journal = {Physical Review C},
   Volume = {75},
   Number = {5},
   Publisher = {American Physical Society (APS)},
   Year = {2007},
   Month = {May},
   url = {http://dx.doi.org/10.1103/physrevc.75.055808},
   Doi = {10.1103/physrevc.75.055808},
   Key = {fds324728}
}

@article{fds324727,
   Author = {Ugalde, C and Champagne, AE and Daigle, S and Iliadis, C and Longland,
             R and Newton, JR and Osenbaugh-Stewart, E and Clark, JA and Deibel, C and Parikh, A and Parker, PD and Wrede, C},
   Title = {Experimental evidence for a natural parity state inMg26and
             its impact on the production of neutrons for
             thesprocess},
   Journal = {Physical Review C},
   Volume = {76},
   Number = {2},
   Publisher = {American Physical Society (APS)},
   Year = {2007},
   Month = {August},
   url = {http://dx.doi.org/10.1103/physrevc.76.025802},
   Doi = {10.1103/physrevc.76.025802},
   Key = {fds324727}
}

@article{fds324726,
   Author = {Gintautas, V and Champagne, AE and Kondev, FG and Longland,
             R},
   Title = {Thermal equilibration ofLu176viaKmixing},
   Journal = {Physical Review C},
   Volume = {80},
   Number = {1},
   Publisher = {American Physical Society (APS)},
   Year = {2009},
   Month = {July},
   url = {http://dx.doi.org/10.1103/physrevc.80.015806},
   Doi = {10.1103/physrevc.80.015806},
   Key = {fds324726}
}

@article{fds324721,
   Author = {Iliadis, C and Longland, R and Champagne, AE and Coc,
             A},
   Title = {Charged-particle thermonuclear reaction rates: III. Nuclear
             physics input},
   Journal = {Nuclear Physics A},
   Volume = {841},
   Number = {1-4},
   Pages = {251-322},
   Publisher = {Elsevier BV},
   Year = {2010},
   Month = {January},
   url = {http://dx.doi.org/10.1016/j.nuclphysa.2010.04.010},
   Abstract = {The nuclear physics input used to compute the Monte Carlo
             reaction rates and probability density functions that are
             tabulated in the second paper of this issue (Paper II) is
             presented. Specifically, we publish the input files to the
             Monte Carlo reaction rate code RatesMC, which is based on
             the formalism presented in the first paper of this issue
             (Paper I). This data base contains overwhelmingly
             experimental nuclear physics information. The survey of
             literature for this review was concluded in November 2009.
             © 2010 Elsevier B.V.},
   Doi = {10.1016/j.nuclphysa.2010.04.010},
   Key = {fds324721}
}

@article{fds324720,
   Author = {Iliadis, C and Longland, R and Champagne, AE and Coc, A and Fitzgerald,
             R},
   Title = {Charged-particle thermonuclear reaction rates: II. Tables
             and graphs of reaction rates and probability density
             functions},
   Journal = {Nuclear Physics A},
   Volume = {841},
   Number = {1-4},
   Pages = {31-250},
   Publisher = {Elsevier BV},
   Year = {2010},
   Month = {January},
   url = {http://dx.doi.org/10.1016/j.nuclphysa.2010.04.009},
   Abstract = {Numerical values of charged-particle thermonuclear reaction
             rates for nuclei in the A=14 to 40 region are tabulated. The
             results are obtained using a method, based on Monte Carlo
             techniques, that has been described in the preceding paper
             of this issue (Paper I). We present a low rate, median rate
             and high rate which correspond to the 0.16, 0.50 and 0.84
             quantiles, respectively, of the cumulative reaction rate
             distribution. The meaning of these quantities is in general
             different from the commonly reported, but statistically
             meaningless expressions, " lower limit" , " nominal value"
             and " upper limit" of the total reaction rate. In addition,
             we approximate the Monte Carlo probability density function
             of the total reaction rate by a lognormal distribution and
             tabulate the lognormal parameters μ and σ at each
             temperature. We also provide a quantitative measure
             (Anderson-Darling test statistic) for the reliability of the
             lognormal approximation. The user can implement the
             approximate lognormal reaction rate probability density
             functions directly in a stellar model code for studies of
             stellar energy generation and nucleosynthesis. For each
             reaction, the Monte Carlo reaction rate probability density
             functions, together with their lognormal approximations, are
             displayed graphically for selected temperatures in order to
             provide a visual impression. Our new reaction rates are
             appropriate for bare nuclei in the laboratory. The nuclear
             physics input used to derive our reaction rates is presented
             in the subsequent paper of this issue (Paper III). In the
             fourth paper of this issue (Paper IV) we compare our new
             reaction rates to previous results. © 2010 Elsevier
             B.V.},
   Doi = {10.1016/j.nuclphysa.2010.04.009},
   Key = {fds324720}
}

@article{fds324723,
   Author = {Iliadis, C and Longland, R and Champagne, AE and Coc,
             A},
   Title = {Charged-particle thermonuclear reaction rates: IV.
             Comparison to previous work},
   Journal = {Nuclear Physics A},
   Volume = {841},
   Number = {1-4},
   Pages = {323-388},
   Publisher = {Elsevier BV},
   Year = {2010},
   Month = {January},
   url = {http://dx.doi.org/10.1016/j.nuclphysa.2010.04.012},
   Abstract = {We compare our Monte Carlo reaction rates (see Paper II of
             this issue) to previous results that were obtained by using
             the classical method of computing thermonuclear reaction
             rates. For each reaction, the comparison is presented using
             two types of graphs: the first shows the change in reaction
             rate uncertainties, while the second displays our new
             results normalized to the previously recommended reaction
             rate. We find that the rates have changed significantly for
             almost all reactions considered here. The changes are caused
             by (i) our new Monte Carlo method of computing reaction
             rates (see Paper I of this issue), and (ii) newly available
             nuclear physics information (see Paper III of this issue).
             © 2010 Elsevier B.V.},
   Doi = {10.1016/j.nuclphysa.2010.04.012},
   Key = {fds324723}
}

@article{fds324725,
   Author = {Newton, JR and Iliadis, C and Champagne, AE and Cesaratto, JM and Daigle, S and Longland, R},
   Title = {Measurement ofO17(p,γ)F18between the narrow resonances
             atErlab=193and519 keV},
   Journal = {Physical Review C},
   Volume = {81},
   Number = {4},
   Publisher = {American Physical Society (APS)},
   Year = {2010},
   Month = {April},
   url = {http://dx.doi.org/10.1103/physrevc.81.045801},
   Doi = {10.1103/physrevc.81.045801},
   Key = {fds324725}
}

@article{fds324724,
   Author = {Longland, R and Iliadis, C and Cesaratto, JM and Champagne, AE and Daigle, S and Newton, JR and Fitzgerald, R},
   Title = {Resonance strength inNe22(p,γ)Na23from depth profiling in
             aluminum},
   Journal = {Physical Review C},
   Volume = {81},
   Number = {5},
   Publisher = {American Physical Society (APS)},
   Year = {2010},
   Month = {May},
   url = {http://dx.doi.org/10.1103/physrevc.81.055804},
   Doi = {10.1103/physrevc.81.055804},
   Key = {fds324724}
}

@article{fds324722,
   Author = {Longland, R and Iliadis, C and Champagne, AE and Newton, JR and Ugalde,
             C and Coc, A and Fitzgerald, R},
   Title = {Charged-particle thermonuclear reaction rates: I. Monte
             Carlo method and statistical distributions},
   Journal = {Nuclear Physics A},
   Volume = {841},
   Number = {1-4},
   Pages = {1-30},
   Publisher = {Elsevier BV},
   Year = {2010},
   Month = {October},
   url = {http://dx.doi.org/10.1016/j.nuclphysa.2010.04.008},
   Abstract = {A method based on Monte Carlo techniques is presented for
             evaluating thermonuclear reaction rates. We begin by
             reviewing commonly applied procedures and point out that
             reaction rates that have been reported up to now in the
             literature have no rigorous statistical meaning.
             Subsequently, we associate each nuclear physics quantity
             entering in the calculation of reaction rates with a
             specific probability density function, including Gaussian,
             lognormal and chi-squared distributions. Based on these
             probability density functions the total reaction rate is
             randomly sampled many times until the required statistical
             precision is achieved. This procedure results in a median
             (Monte Carlo) rate which agrees under certain conditions
             with the commonly reported recommended " classical" rate. In
             addition, we present at each temperature a low rate and a
             high rate, corresponding to the 0.16 and 0.84 quantiles of
             the cumulative reaction rate distribution. These quantities
             are in general different from the statistically meaningless
             " minimum" (or " lower limit" ) and " maximum" (or " upper
             limit" ) reaction rates which are commonly reported.
             Furthermore, we approximate the output reaction rate
             probability density function by a lognormal distribution and
             present, at each temperature, the lognormal parameters μ
             and σ. The values of these quantities will be crucial for
             future Monte Carlo nucleosynthesis studies. Our new reaction
             rates, appropriate for bare nuclei in the laboratory, are
             tabulated in the second paper of this issue (Paper II). The
             nuclear physics input used to derive our reaction rates is
             presented in the third paper of this issue (Paper III). In
             the fourth paper of this issue (Paper IV) we compare our new
             reaction rates to previous results. © 2010 Elsevier
             B.V.},
   Doi = {10.1016/j.nuclphysa.2010.04.008},
   Key = {fds324722}
}

@article{fds324719,
   Author = {Cesaratto, JM and Champagne, AE and Clegg, TB and Buckner, MQ and Runkle, RC and Stefan, A},
   Title = {Nuclear astrophysics studies at LENA: The
             accelerators},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {623},
   Number = {3},
   Pages = {888-894},
   Publisher = {Elsevier BV},
   Year = {2010},
   Month = {November},
   url = {http://dx.doi.org/10.1016/j.nima.2010.08.104},
   Doi = {10.1016/j.nima.2010.08.104},
   Key = {fds324719}
}

@article{fds324718,
   Author = {Oginni, BM and Iliadis, C and Champagne, AE},
   Title = {Theoretical evaluation of the reaction rates
             forAl26(n,p)26Mg andAl26(n,α)23Na},
   Journal = {Physical Review C},
   Volume = {83},
   Number = {2},
   Publisher = {American Physical Society (APS)},
   Year = {2011},
   Month = {February},
   url = {http://dx.doi.org/10.1103/physrevc.83.025802},
   Doi = {10.1103/physrevc.83.025802},
   Key = {fds324718}
}

@article{fds324717,
   Author = {Buckner, MQ and Iliadis, C and Cesaratto, JM and Howard, C and Clegg,
             TB and Champagne, AE and Daigle, S},
   Title = {Thermonuclear reaction rate of18O(p,γ)19F},
   Journal = {Physical Review C},
   Volume = {86},
   Number = {6},
   Publisher = {American Physical Society (APS)},
   Year = {2012},
   Month = {December},
   url = {http://dx.doi.org/10.1103/physrevc.86.065804},
   Doi = {10.1103/physrevc.86.065804},
   Key = {fds324717}
}

@article{fds324716,
   Author = {Howard, C and Iliadis, C and Champagne, A},
   Title = {Monte Carlo simulation of the LENA detector
             system},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {729},
   Pages = {254-259},
   Year = {2013},
   Month = {November},
   url = {http://dx.doi.org/10.1016/j.nima.2013.07.032},
   Doi = {10.1016/j.nima.2013.07.032},
   Key = {fds324716}
}

@article{fds324715,
   Author = {Cesaratto, JM and Champagne, AE and Buckner, MQ and Clegg, TB and Daigle, S and Howard, C and Iliadis, C and Longland, R and Newton, JR and Oginni, BM},
   Title = {Measurement of theErc.m.=138keV resonance in
             the23Na(p,γ)24Mg reaction and the abundance of sodium in
             AGB stars},
   Journal = {Physical Review C},
   Volume = {88},
   Number = {6},
   Publisher = {American Physical Society (APS)},
   Year = {2013},
   Month = {December},
   url = {http://dx.doi.org/10.1103/physrevc.88.065806},
   Doi = {10.1103/physrevc.88.065806},
   Key = {fds324715}
}

@article{fds324714,
   Author = {Champagne, AE and Iliadis, C and Longland, R},
   Title = {Nuclear astrophysics in the laboratory and in the
             universe},
   Journal = {Aip Advances},
   Volume = {4},
   Number = {4},
   Pages = {041006-041006},
   Year = {2014},
   Month = {April},
   url = {http://dx.doi.org/10.1063/1.4864794},
   Doi = {10.1063/1.4864794},
   Key = {fds324714}
}

@article{fds324713,
   Author = {Buckner, MQ and Iliadis, C and Kelly, KJ and Downen, LN and Champagne,
             AE and Cesaratto, JM and Howard, C and Longland, R},
   Title = {High-intensity-beam study ofO17(p,γ)F18and thermonuclear
             reaction rates forO17+p},
   Journal = {Physical Review C},
   Volume = {91},
   Number = {1},
   Publisher = {American Physical Society (APS)},
   Year = {2015},
   Month = {January},
   url = {http://dx.doi.org/10.1103/physrevc.91.015812},
   Doi = {10.1103/physrevc.91.015812},
   Key = {fds324713}
}

@article{fds324712,
   Author = {Iliadis, C and Longland, R and Coc, A and Timmes, FX and Champagne,
             AE},
   Title = {Statistical methods for thermonuclear reaction rates and
             nucleosynthesis simulations},
   Journal = {Journal of Physics G: Nuclear and Particle
             Physics},
   Volume = {42},
   Number = {3},
   Pages = {034007-034007},
   Publisher = {IOP Publishing},
   Year = {2015},
   Month = {March},
   url = {http://dx.doi.org/10.1088/0954-3899/42/3/034007},
   Doi = {10.1088/0954-3899/42/3/034007},
   Key = {fds324712}
}

@article{fds324711,
   Author = {deBoer, RJ and Bardayan, DW and Görres, J and LeBlanc, PJ and Manukyan,
             KV and Moran, MT and Smith, K and Tan, W and Uberseder, E and Wiescher, M and Bertone, PF and Champagne, AE and Islam, MS},
   Title = {Low energy scattering cross section ratios
             ofN14(p,p)N14},
   Journal = {Physical Review C},
   Volume = {91},
   Number = {4},
   Publisher = {American Physical Society (APS)},
   Year = {2015},
   Month = {April},
   url = {http://dx.doi.org/10.1103/physrevc.91.045804},
   Doi = {10.1103/physrevc.91.045804},
   Key = {fds324711}
}

@article{fds324710,
   Author = {Howard, C and Daigle, S and Buckner, M and Erikson, LE and Runkle, RC and Stave, SC and Champagne, AE and Cooper, A and Downen, L and Glasgow, BD and Kelly, K and Sallaska, A},
   Title = {Performance of a compact multi-crystal high-purity germanium
             detector array for measuring coincident gamma-ray
             emissions},
   Journal = {Nuclear Instruments and Methods in Physics Research Section
             A: Accelerators, Spectrometers, Detectors and Associated
             Equipment},
   Volume = {783},
   Pages = {85-94},
   Year = {2015},
   Month = {May},
   url = {http://dx.doi.org/10.1016/j.nima.2015.02.022},
   Doi = {10.1016/j.nima.2015.02.022},
   Key = {fds324710}
}

@article{fds324709,
   Author = {Kelly, KJ and Champagne, AE and Longland, R and Buckner,
             MQ},
   Title = {New recommended ωγ for the Er c. m. =458 keV resonance in
             Ne 22 (p,γ) Na 23},
   Journal = {Physical Review C},
   Volume = {92},
   Number = {3},
   Publisher = {American Physical Society (APS)},
   Year = {2015},
   Month = {September},
   url = {http://dx.doi.org/10.1103/PhysRevC.92.035805},
   Abstract = {© 2015 American Physical Society. ©2015 American Physical
             Society. The Erc.m.=458 keV resonance in Ne22(p,γ)Na23 is
             an ideal reference resonance for measurements of cross
             sections and resonance strengths in noble gas targets. We
             report on a new measurement of the strength of this
             resonance. Data analysis employed the TFractionFitter class
             of root combined with geant simulations of potential decay
             cascades from this resonance. This approach allowed us to
             extract precise primary branching ratios for decays from the
             resonant state, including a new primary branch to the
             7082-keV state in Na23. Our new resonance strength of
             ωγ(458 keV) = 0.583(43) eV is more than 1σ higher than a
             recent high-precision result that relied on literature
             branching ratios.},
   Doi = {10.1103/PhysRevC.92.035805},
   Key = {fds324709}
}

@article{fds324708,
   Author = {Daigle, S and Kelly, KJ and Champagne, AE and Buckner, MQ and Iliadis,
             C and Howard, C},
   Title = {Measurement of theErc.m.=259 keV resonance in
             theN14(p,γ)O15reaction},
   Journal = {Physical Review C},
   Volume = {94},
   Number = {2},
   Publisher = {American Physical Society (APS)},
   Year = {2016},
   Month = {August},
   url = {http://dx.doi.org/10.1103/physrevc.94.025803},
   Doi = {10.1103/physrevc.94.025803},
   Key = {fds324708}
}