THESE de DOCTORAT Lyu ABE Imagerie à Haute Dynamique ...

236 Bibliographie[49] Fordham J. L. A., Moorhead C. F., Galbraith R. F., "Dynamic range limitations of intensified CCDphoton counting detectors" (2000), MNRAS, vol.312, p.83-88[50] Foy R., "The photon counting camera CP40" (1988), Instrumentation for Ground-Based OpticalAstronomy, Present and Future, Eds. L. B. Robinson, Publisher, Springer-Verlag, New York, NY,p.589[51] Fried D. L., "Limiting Resolution Looking Down Through the Atmosphere" (1966), J. Opt. Soc.Am., vol.56, p.1372[52] Gay J., Rabbia Y., "Principe d’un coronographe interférentiel" (1996), Comptes Rendus de l’Académiedes Sciences Paris, tome 332, Série II, p. 265-271[53] Germain M. E., "Intensified CCD Fringe Tracker" (1999), SPIE proc., vol.4006, p.1029-1034[54] Glindemann A., Rees N. P., "Photon counting versus CCD sensors for wavefront sensing : performancecomparison in the presence of noise" (1994), Proc. SPIE, vol.2199, p. 824-834[55] Guillot T. & Showman A. P., "Evolution of "51 Pegasus b-like" planets" (2002), A&A, vol.385,p.156[56] Guyon O., Roddier C., Graves J. E., Roddier F., Cuevas S., Espejo C., Gonzalez S., MartinezA., Bisiacchi G., Vuntesmeri V., "The Nulling Stellar Coronagraph : Laboratory Tests and PerformanceEvaluation" (1999), PASP, vol.111, p.1321[57] Hoffmann K. H., Mauder W. & Weigelt G., "Photon-Counting speckle imaging" (1990), Proc. Soc.Photo-Opt. Instrum. Eng., vol.1319, p.442-443[58] Hoffmann K. H., "Photon-Counting speckle imaging : the photon-counting hole in triple correlation"(1993), J. Opt. Soc. Am. A., vol.10 (2), p.329-335[59] Janesick J., "Lux transfer : CMOS versus CCD" (2002)[60] Jerram P. , Pool P., Bell R., Burt D., Bowring S., Spencer S., Hazelwood M., Moody I., CatlettN., Heyes P. "The LLLCCD : Low Light Imaging without the need for an intensifier" (2000), MarconiApplied Technologies, Chelmsford, Essex, UK[61] Keller C. U., Graff W., Rosselet A., Gschwind R., Wild U. P., "First light for an astronomical 3-Dphoton detector" (1994), A&A, vol.289, p.L41[62] Keller C. U., Gschwind R., Renn A., Rosselet A., Wild U. P., "The spectral hole-burning device :a 3-dimensional photon detector" (1995), A&AS Ser., vol.109, p.383[63] Koechlin L., "Développement et exploitation astrophysique de l’interférométre à deux télescopesdu CERGA" (1985), Thèse de doctorat d’état[64] Koechlin L., "Dispersed fringe tracking with the multi-ro apertures of the Grand Interféromètre à 2Télescopes" (1996), Applied Optics, vol.35, Issue 16, June 1, 1996, pp.3002-3009[65] Kuhn J. R., Hawley S. L., "Some astronomical performance advantages of off-axis telescopes"(1999), PASP, vol.111, p.601-620[66] Labeyrie A., "Attainment of Diffraction Limited Resolution in Large Telescopes by Fourier AnalysingSpeckle Patterns in Star Images" (1970), A&A, vol.6, p.85