PI: Daniel Bemmerer and Antonio Caciolli

WG members: D. Bemmerer, C. Broggini, A. Caciolli, F. Cavanna, R. Depalo, Z. Elekes, F. Ferraro, G. Gervino, A. Guglielmetti, I. Kochanek, P. Marigo, R. Menegazzo, D. Piatti, P. Prati, O. Straniero, T. Szuecs, M. Takacs, D. Trezzi

 

Astrophysical Motivation:

  • nucleosinthesys in Ne-Na cycle

  • nova, AGB, and supernova nucleosinthesys

  • direct observation of several resonances below Ep = 400 keV

 

Documentation