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Volumn 49, Issue 31, 2010, Pages

Low-light-level charge-coupled devices for pyramid wavefront sensing on 8 m class telescopes: What actual gain?

Author keywords

[No Author keywords available]

Indexed keywords

CHARGE COUPLED DEVICES; LIGHT; POISSON DISTRIBUTION; TELESCOPES; WAVEFRONTS;

EID: 78149433339     PISSN: 1559128X     EISSN: 15394522     Source Type: Journal    
DOI: 10.1364/AO.49.00G167     Document Type: Article
Times cited : (9)

References (16)
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    • 0000465737 scopus 로고    scopus 로고
    • Pupil plane wavefront sensing with an oscillating prism
    • R. Ragazzoni, "Pupil plane wavefront sensing with an oscillating prism," J. Mod. Opt. 43, 289-293 (1996).
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    • Ragazzoni, R.1
  • 10
    • 0001329336 scopus 로고    scopus 로고
    • Sensitivity of a pyramidic wave-front sensor in closed loop adaptive optics
    • R. Ragazzoni and J. Farinato, "Sensitivity of a pyramidic wave-front sensor in closed loop adaptive optics," Astron. Astrophys. 350, L23-L26 (1999).
    • (1999) Astron. Astrophys. , vol.350
    • Ragazzoni, R.1    Farinato, J.2
  • 11
    • 0035298218 scopus 로고    scopus 로고
    • Pyramid wavefront sensor behavior in partial correction adaptive optics systems
    • S. Esposito and A. Riccardi, "Pyramid wavefront sensor behavior in partial correction adaptive optics systems," Astron. Astrophys. 369,L9-L12 (2001).
    • (2001) Astron. Astrophys. , vol.369
    • Esposito, S.1    Riccardi, A.2
  • 12
    • 25144459188 scopus 로고    scopus 로고
    • Adaptive optics for high-contrast imaging: Pyramid sensor versus Shack-Hartmann sensor
    • C. Vérinaud, M. Le Louarn, V. Korkiakoski, and M. Carbillet, "Adaptive optics for high-contrast imaging: pyramid sensor versus Shack-Hartmann sensor," Mon. Not. R. Astron. Soc. 357, L26-L30 (2005).
    • (2005) Mon. Not. R. Astron. Soc. , vol.357
    • Vérinaud, C.1    Le Louarn, M.2    Korkiakoski, V.3    Carbillet, M.4
  • 15
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    • Numerical modeling of atmospherically perturbed phase screens: New solutions for classical fast Fourier transform and Zernike methods
    • M. Carbillet and A. Riccardi, "Numerical modeling of atmospherically perturbed phase screens: new solutions for classical fast Fourier transform and Zernike methods," Appl. Opt. 49, G47-G52 (2010).
    • (2010) Appl. Opt. , vol.49
    • Carbillet, M.1    Riccardi, A.2
  • 16
    • 11144324899 scopus 로고    scopus 로고
    • Numerical simulation studies for the first-light adaptive optics system of the Large Binocular Telescope
    • M. Carbillet, A. Riccardi, and S. Esposito, "Numerical simulation studies for the first-light adaptive optics system of the Large Binocular Telescope," Proc. SPIE 5490, 731-732 (2004).
    • (2004) Proc. SPIE , vol.5490 , pp. 731-732
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.