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Number of items: 4.

Goldblum, B. L. and Wiedeking, M. and Reed, T. and Alfonso, K. and Allmond, J. M. and Bernstein, L. A. and Bleuel, D. L. and Dietrich, F. S. and Hatarik, R. and Lake, P. T. and Lee, I.-Y. and Lesher, S. R. and Paschalis, S. and Petri, Marina and Phair, L. and Scielzo, N. D. and Vial, R. and Vujic, J. (2012):
Indirect determination of neutron capture cross sections on spherical and near-spherical nuclei using the surrogate method.
In: Physical Review C, 85, (5), ISSN 0556-2813,
[Online-Edition: http://dx.doi.org/10.1103/PhysRevC.85.054616],
[Article]

Church, J. A. and Ahle, L. and Bernstein, L. A. and Cooper, J. and Dietrich, F. S. and Escher, J. and Forssén, C. and Ai, H. and Amro, H. and Babilon, Mario and Beausang, C. and Caggiano, J. and Heinz, A. and Hughes, R. and McCutchan, E. and Meyer, D. and Plettner, Cristina and Ressler, J. and Zamfir, V. (2005):
Determining neutron capture cross sections with the Surrogate Reaction Technique: Measuring decay probabilities with STARS.
In: Nucl. Phys. A, pp. 126c, 758, [Article]

Church, J. A. and Ahle, L. and Bernstein, L. A. and Cooper, J. and Dietrich, F. S. and Escher, J. and Forssén, C. and Ai, H. and Amro, H. and Babilon, M. and Beausang, C. and Caggiano, J. and Heinz, A. and Hughes, R. and McCutchan, E. and Meyer, D. and Plettner, C. and Ressler, J. and Zamfir, V. (2005):
Determining neutron capture cross sections with the Surrogate Reaction Technique: Measuring decay probabilities with STARS.
In: Nuclear Physics A, p. 126, 758, ISSN 03759474,
[Online-Edition: http://dx.doi.org/10.1016/j.nuclphysa.2005.05.169],
[Article]

Church, J. A. and Ahle, L. and Bernstein, L. A. and Cooper, J. and Dietrich, F. S. and Escher, J. and Forssén, C. and Ai, H. and Amro, H. and Babilon, Mario and Beausang, C. and Caggiano, J. and Heinz, A. and Hughes, R. and McCutchan, E. and Meyer, D. and Plettner, Cristina and Ressler, J. J. and Zamfir, V. (2005):
Determining neutron capture cross sections with the surrogate reaction technique : measuring decay probabilities with STARS.
In: Nuclear Physics A, pp. 126c, 758, [Article]

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