Thermonuclear 42Ti(p,gamma)43V rate in type I X-ray bursts
  The thermonuclear rate of the $^{42}$Ti($p$,$\gamma$)$^{43}$V reaction has been reevaluated based on a recent precise proton separation energy measurement of $S_p$($^{43}$V)=83$\pm$43 keV. The astrophysical impact of our new rates has been investigated through one-zone postprocessing type I x-ray burst calculations. It shows that the new experimental value of $S_p$ significantly affects the yields of species between A$\approx$40--45. As well, the precision of the recent experimental $S_p$ value constrains these yields to better than a factor of three. 
J.J. He, A. Parikh, B.A. Brown, T. Rauscher, S.Q. Hou, Y.H. Zhang,   X.H. Zhou, H.S. Xu
nucl-th