Resonance Strength Measurement at Astrophysical Energies: The 17O(p,α)14N Reaction Studied via THM by Sergi M.L., Spitaleri C., La Cognata M., Lamia L., Pizzone R.G., Rapisarda G.G., Mukhamedzhanov A., Irgaziev B., Tang X.D., Wischer M., Mrazek J., Kroha V.

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The astrophysical S-factor of the direct 18O(p, γ)19F capture by the ANC method by Burjan V., Hons Z., Kroha V., Mrázek J., Piskoř Š., Mukhamedzhanov A. M., Trache L., Tribble R. E., La Cognata M., Lamia L., Pizzone G. R., Romano S., Spitaleri C., Tumino A.

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ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case by D’Agata G., Kilic A. I., Burjan V., Mrázek J., Glagolev V., Kroha V., Cassisa A., Guardo G. L., La Cognata M., Lamia L., Palmerini S., Pizzone R. G., Rapisarda G. G., Romano S., Sergi M. L., Spartà R., Spitaleri C., Tumino A.

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Spectator invariance test in the study of the Trojan Horse Method 6,7Li fusion reactions via the Trojan Horse Method by Li C., La Cognata M., Kroha V., Kiss G.G., Hons Z., Cherubini S., Burjan V., Blokhintsev L., Spitaleri C., Mukhamedzhanov A., Bertulani C., Lamia L., Pizzone R.G., Mrazek J., Piskoř S., Puglia S.M.R., Rapisarda G.G., Romano S., Sergi M.L., Tumino A.

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