© 2006 Optical Society of America

1. J. Schneider, The Extrasolar Planets Encyclopaedia, Tech. rep. (CNRS-LUTH, Paris Observatory, 2006), http://vo.obspm.fr/exoplanetes/encyclo/catalog.php.
2. L. A. Poyneer and B. Macintosh, "Spatially filtered wave-front sensor for high-order adaptive optics," J. Opt. Soc. Am. A 21, 810-819 (2004). [CrossRef]
3. L. A. Poyneer and J.-P. Véran, "Optimal modal Fourier transform wave-front control," J. Opt. Soc. Am. A 22, 1515-1526 (2005). [CrossRef]
4. M. D. Perrin, A. Sivaramakrishnan, R. B. Makidon, B. R. Oppenheimer, and J. R. Graham, "The structure of high Strehl ratio point-spread functions," Astrophys. J. 596, 702-712 (2003). [CrossRef]
5. L. A. Poyneer, D. T. Gavel, and J. M. Brase, "Fast wavefront reconstruction in large adaptive optics systems with use of the Fourier transform," J. Opt. Soc. Am. A 19, 2100-2111 (2002). [CrossRef]
6. E. Gendron and P. Léna, "Astronomical adaptive optics, 1: Modal control optimization," Astron. Astrophys. 291, 337-347 (1994).
7. P.-Y. Madec, "Control Techniques," in Adaptive Optics in Astronomy, F. Roddier, ed. (Cambridge University Press, 1999) pp. 131-154.
8. A. Tokovinin, "Modeling turbulence profile for GLAO," Tech. rep. (Gemini Observatory, 2004).
9. E. M. Johansson and D. T. Gavel, "Simulation of stellar speckle imaging," in Amplitude and Intensity Spatial Interferometry II, J. B. Breckinridge, ed., Proc. SPIE 1237 (1994) pp. 372-383. [CrossRef]
10. S. B. Howell, Handbook of CCD Astronomy (Cambridge University Press, 2000).
11. J. J. Green and S. B. Shaklan, "Optimizing coronagraph designs to minimize their contrast sensitivity to loworder optical aberrations," in Techniques and Instrumentation for Detection of Exoplanets, D. R. Coulter, ed., Proc. SPIE 5170 (2003) pp. 25-37. [CrossRef]
12. B. L. Ellerbroek, "Linear systems modeling of adaptive optics in the spatial-frequency domain," J. Opt. Soc. Am. A 22, 310-322 (2005). [CrossRef]
13. L. Jolissaint, J.-P. Véran, and R. Conan, "Analytical modeling of adaptive optics: foundations of the phase spatial power spectrum approach," J. Opt. Soc. Am. A 23, 382-394 (2006). [CrossRef]
14. C. Aime and R. Soummer, "The usefulness and limits of coronagraphy in the presence of pinned speckles," Astrophys. J. 612, L85-L88 (2004). [CrossRef]
15. M. P. Fitzgerald and J. R. Graham, "Speckle statistics in adaptively corrected images," Astrophys. J. 637, 541-547 (2006). [CrossRef]
16. R. Racine, G. A. H. Walker, D. Nadeau, R. Doyon, and C. Marois, "Speckle noise and the detection of faint companions," Publ. Astron. Soc. Pac. 111, 587-594 (1999). [CrossRef]
17. B. Macintosh, L. A. Poyneer, A. Sivaramakrishnan, and C. Marois, "Speckle lifetimes in high-contrast adaptive optics," in Astronomical Adaptive Optics Systems and Applications II, R. K. Tyson andM. Llyod-Hart, eds., Proc. SPIE 5903 (2005) p. 59030J. [CrossRef]
18. A. V. Oppenheim, R. W. Schafer, and J. R. Buck, Discrete-time Signal Processing (Prentice Hall, 1999).

Astron. Astrophys.

• E. Gendron and P. Léna, "Astronomical adaptive optics, 1: Modal control optimization," Astron. Astrophys. 291, 337-347 (1994).

Astrophys. J.

• M. D. Perrin, A. Sivaramakrishnan, R. B. Makidon, B. R. Oppenheimer, and J. R. Graham, "The structure of high Strehl ratio point-spread functions," Astrophys. J. 596, 702-712 (2003). [CrossRef]
• C. Aime and R. Soummer, "The usefulness and limits of coronagraphy in the presence of pinned speckles," Astrophys. J. 612, L85-L88 (2004). [CrossRef]
• M. P. Fitzgerald and J. R. Graham, "Speckle statistics in adaptively corrected images," Astrophys. J. 637, 541-547 (2006). [CrossRef]

J. Opt. Soc. Am. A

• B. L. Ellerbroek, "Linear systems modeling of adaptive optics in the spatial-frequency domain," J. Opt. Soc. Am. A 22, 310-322 (2005). [CrossRef]
• L. Jolissaint, J.-P. Véran, and R. Conan, "Analytical modeling of adaptive optics: foundations of the phase spatial power spectrum approach," J. Opt. Soc. Am. A 23, 382-394 (2006). [CrossRef]
• L. A. Poyneer, D. T. Gavel, and J. M. Brase, "Fast wavefront reconstruction in large adaptive optics systems with use of the Fourier transform," J. Opt. Soc. Am. A 19, 2100-2111 (2002). [CrossRef]
• L. A. Poyneer and B. Macintosh, "Spatially filtered wave-front sensor for high-order adaptive optics," J. Opt. Soc. Am. A 21, 810-819 (2004). [CrossRef]
• L. A. Poyneer and J.-P. Véran, "Optimal modal Fourier transform wave-front control," J. Opt. Soc. Am. A 22, 1515-1526 (2005). [CrossRef]

Publ. Astron. Soc. Pac.

• R. Racine, G. A. H. Walker, D. Nadeau, R. Doyon, and C. Marois, "Speckle noise and the detection of faint companions," Publ. Astron. Soc. Pac. 111, 587-594 (1999). [CrossRef]

Other

• B. Macintosh, L. A. Poyneer, A. Sivaramakrishnan, and C. Marois, "Speckle lifetimes in high-contrast adaptive optics," in Astronomical Adaptive Optics Systems and Applications II, R. K. Tyson andM. Llyod-Hart, eds., Proc. SPIE 5903 (2005) p. 59030J. [CrossRef]
• A. V. Oppenheim, R. W. Schafer, and J. R. Buck, Discrete-time Signal Processing (Prentice Hall, 1999).
• J. Schneider, The Extrasolar Planets Encyclopaedia, Tech. rep. (CNRS-LUTH, Paris Observatory, 2006), http://vo.obspm.fr/exoplanetes/encyclo/catalog.php.
• P.-Y. Madec, "Control Techniques," in Adaptive Optics in Astronomy, F. Roddier, ed. (Cambridge University Press, 1999) pp. 131-154.
• A. Tokovinin, "Modeling turbulence profile for GLAO," Tech. rep. (Gemini Observatory, 2004).
• E. M. Johansson and D. T. Gavel, "Simulation of stellar speckle imaging," in Amplitude and Intensity Spatial Interferometry II, J. B. Breckinridge, ed., Proc. SPIE 1237 (1994) pp. 372-383. [CrossRef]
• S. B. Howell, Handbook of CCD Astronomy (Cambridge University Press, 2000).
• J. J. Green and S. B. Shaklan, "Optimizing coronagraph designs to minimize their contrast sensitivity to loworder optical aberrations," in Techniques and Instrumentation for Detection of Exoplanets, D. R. Coulter, ed., Proc. SPIE 5170 (2003) pp. 25-37. [CrossRef]

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