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M. J. Kuchner and W. A. Traub, A Coronagraph with a Band???limited Mask for Finding Terrestrial Planets, The Astrophysical Journal, vol.570, issue.2, p.900, 2002.
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F. Allard, The Limiting Effects of Dust in Brown Dwarf Model Atmospheres, The Astrophysical Journal, vol.556, issue.1, p.357, 2001.
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R. Aime and C. , Principle of an Achromatic Prolate Apodized Lyot Coronagraph, Publications of the Astronomical Society of the Pacific, vol.117, issue.835, p.1012, 2005.
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C. Cavarroc, A. Boccaletti, P. Baudoz, T. Fusco, and D. Rouan, Fundamental limitations on Earth-like planet detection with extremely large telescopes, Astronomy and Astrophysics, vol.447, issue.1, p.397, 2006.
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O. Guyon, Imaging Faint Sources within a Speckle Halo with Synchronous Interferometric Speckle Subtraction, The Astrophysical Journal, vol.615, issue.1, p.562, 2004.
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M. J. Kuchner and W. A. Traub, A Coronagraph with a Band???limited Mask for Finding Terrestrial Planets, The Astrophysical Journal, vol.570, issue.2, p.900, 2002.
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B. Macintosh, J. Graham, and D. Palmer, Presented at the Society of Photo-Optical Instrumentation Engineers, Advances in Adaptive Optics II Proc. SPIE Conf, p.91, 2000.

D. Mawet, P. Riaud, O. Absil, and J. Surdej, Annular Groove Phase Mask Coronagraph, The Astrophysical Journal, vol.633, issue.2, p.1191, 2005.
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J. Nelson and G. H. Sanders, in Ground-based and Airborne Telescopes, Presented at the Society of Photo-Optical Instrumentation Engineers, Proc. SPIE Conf, p.626728, 2006.

R. Racine, G. A. Walker, D. Nadeau, R. Doyon, and C. Marois, Speckle Noise and the Detection of Faint Companions, Publications of the Astronomical Society of the Pacific, vol.111, issue.759, p.587, 1999.
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F. Roddier and C. Roddier, Stellar Coronograph with Phase Mask, Publications of the Astronomical Society of the Pacific, vol.109, p.815, 1997.
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D. Rouan, P. Riaud, A. Boccaletti, Y. Clénet, and A. Labeyrie, The Four???Quadrant Phase???Mask Coronagraph. I. Principle, Publications of the Astronomical Society of the Pacific, vol.112, issue.777, p.1479, 2000.
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