“…[13], the 16 O( 3 He, d) 17 F reaction was measured to analyze the states of 17 F and the deduced ANCs were then used to determine the low energy radiative capture cross sections of the 16 O(p, γ) 17 F reaction. Similarly, the cluster transfer reactions such as ( 6 Li, d) and ( 7 Li, t), where an α cluster transfer from the projectile to the target, have been used to study the important astrophysical reactions like 12 C(α, γ) 16 O, 13 C(α, n) 16 O, 22 Ne(α, γ) 26 Mg, (for details see for example the review article [10]). It is now well established that cross sections of low energy peripheral radiative capture reactions are mainly determine by the ANCs.…”