LIMITS OF ADAPTIVE OPTICS FOR HIGH-CONTRAST IMAGING
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[1] W. Talbot. Facts relating to optical science , 1836 .
[2] F. Zernike,et al. Diffraction Theory of the Knife-Edge Test and its Improved Form, The Phase-Contrast Method , 1934 .
[3] B. Edĺen. The Refractive Index of Air , 1966 .
[4] R. Gerchberg. A practical algorithm for the determination of phase from image and diffraction plane pictures , 1972 .
[5] C. G. Wyne. Extending the bandwidth of speckle interferometry , 1979 .
[6] F. Roddier,et al. Twin-image holography with spectrally broad light , 1980 .
[7] F Roddier,et al. Curvature sensing and compensation: a new concept in adaptive optics. , 1988, Applied optics.
[8] Farrokh Vakili,et al. Beam Combination In Aperture Synthesis From Space: Field Of View Limitations And (U,V) Plane Coverage Optimization , 1989, Other Conferences.
[9] F. Roddier,et al. A SIMPLE LOW-ORDER ADAPTIVE OPTICS SYSTEM FOR NEAR-INFRARED APPLICATIONS , 1991 .
[10] J. Angel,et al. Ground-based imaging of extrasolar planets using adaptive optics , 1994, Nature.
[11] Brent L. Ellerbroek,et al. Profiles of nighttime turbulence above Mauna Kea and isoplanatism extension in adaptive optics , 1995, Optics & Photonics.
[12] M. Shao,et al. HIGH-DYNAMIC-RANGE IMAGING USING A DEFORMABLE MIRROR FOR SPACE CORONOGRAPHY , 1995, astro-ph/9502042.
[13] J R Leger,et al. Optical antialiasing filters based on complementary Golay codes. , 1997, Applied optics.
[14] F. Roddier,et al. STELLAR CORONOGRAPH WITH PHASE MASK , 1997 .
[15] C. Moutou,et al. PRESENT PERFORMANCE OF THE DARK-SPECKLE CORONAGRAPH , 1998 .
[16] J. Hardy,et al. Adaptive Optics for Astronomical Telescopes , 1998 .
[17] Gordon A. H. Walker,et al. Speckle Noise and the Detection of Faint Companions , 1999 .
[18] A. Labeyrie,et al. The Four-Quadrant Phase-Mask Coronagraph. I. Principle , 2000 .
[19] P. Baudoz,et al. Achromatic interfero coronagraphy I. Theoretical capabilities for ground-based observations , 2000 .
[20] C. Marois,et al. Efficient Speckle Noise Attenuation in Faint Companion Imaging , 2000 .
[21] Eric E. Bloemhof,et al. Behavior of Remnant Speckles in an Adaptively Corrected Imaging System , 2001 .
[22] D. Spergel,et al. Notch-Filter Masks: Practical Image Masks for Planet-finding Coronagraphs , 2002, astro-ph/0209271.
[23] R. Paul Butler,et al. Scientific Frontiers in Research on Extrasolar Planets , 2003 .
[24] C. Aime,et al. Stellar coronagraphy with prolate apodized circular apertures , 2003 .
[25] J. K. Wallace,et al. Phase contrast techniques for wavefront sensing and calibration in adaptive optics , 2003, SPIE Optics + Photonics.
[26] Roberto Gilmozzi,et al. Critical science for the largest telescopes: science drivers for a 100m ground-based optical-IR telescope , 2003, SPIE Astronomical Telescopes + Instrumentation.
[27] C. Aime,et al. Achromatic dual-zone phase mask stellar coronagraph , 2003 .
[28] B. Krauskopf,et al. Proc of SPIE , 2003 .
[29] R. Vanderbei,et al. Extrasolar Planet Finding via Optimal Apodized-Pupil and Shaped-Pupil Coronagraphs , 2003 .
[30] Eric E. Bloemhof. Suppression of Speckle Noise by Speckle Pinning in Adaptive Optics , 2003 .
[31] GROUND-BASED NEAR-INFRARED IMAGING OF THE HD 141569 CIRCUMSTELLAR DISK , 2002, astro-ph/0211648.
[32] Michael C. B. Ashley,et al. Exceptional astronomical seeing conditions above Dome C in Antarctica , 2004, Nature.
[33] Olivier Guyon,et al. Imaging Faint Sources within a Speckle Halo with Synchronous Interferometric Speckle Subtraction , 2004 .
[34] Claude Aime,et al. The Usefulness and Limits of Coronagraphy in the Presence of Pinned Speckles , 2004 .
[35] Roberto Gilmozzi. Science and technology drivers for future giant telescopes , 2004, SPIE Astronomical Telescopes + Instrumentation.
[36] A. Kostinski,et al. One-sided Achromatic Phase Apodization for Imaging of Extrasolar Planets , 2004 .
[37] Christophe Verinaud,et al. On the nature of the measurements provided by a pyramid wave-front sensor , 2004 .
[38] S. Ridgway,et al. Exoplanet Imaging with a Phase-induced Amplitude Apodization Coronagraph. I. Principle , 2004, astro-ph/0412179.
[39] Johanan L. Codona,et al. Imaging extrasolar planets by stellar halo suppression in separately corrected color bands , 2004 .
[40] B. Macintosh,et al. Spatially filtered wave-front sensor for high-order adaptive optics. , 2004, Journal of the Optical Society of America. A, Optics, image science, and vision.
[41] Mark Chun,et al. Optical Turbulence Profiles at Mauna Kea Measured by MASS and SCIDAR , 2005 .
[42] C. Vérinaud,et al. Adaptive optics for high‐contrast imaging: pyramid sensor versus spatially filtered Shack–Hartmann sensor , 2005 .