S Esposito1, E Pinna, A Puglisi
1Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125-Firenze, Italy. esposito@arcetri.astro.it
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This study demonstrates a pyramid wavefront sensor for aligning segmented mirrors, achieving a 10 nm residual error. This technique is promising for phasing large astronomical telescopes.
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