Paper
7 February 2003 Photon counting CCDs as wavefront sensors for A.O.
Italo Foppiani, Carlo Baffa, Valdemaro Biliotti, G. Bregoli, G. Cosentino, Elizabetta Giani, Simone Esposito, Bruno Marano, Piero Salinari
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Abstract
Limiting magnitude of A.O. reference stars is set by wavefront sensor intrinsic noise. Recently available avalanche intensified CCD detectors allow single photon event detection (photon counting) virtually free from readout noise. The paper describes a program started in spring 2002, aiming to use a Marconi L3CCD as a wavefront sensor for A.O.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Italo Foppiani, Carlo Baffa, Valdemaro Biliotti, G. Bregoli, G. Cosentino, Elizabetta Giani, Simone Esposito, Bruno Marano, and Piero Salinari "Photon counting CCDs as wavefront sensors for A.O.", Proc. SPIE 4839, Adaptive Optical System Technologies II, (7 February 2003); https://doi.org/10.1117/12.478387
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CITATIONS
Cited by 5 scholarly publications.
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KEYWORDS
Charge-coupled devices

Sensors

Wavefront sensors

Stars

CCD image sensors

Photon counting

Electrons

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