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

More documents

Recommendations

Info

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
Bibliographie 237[67] Labeyrie A., "Interference fringes obtained on VEGA with two optical telescopes" (1975), AstrophysicalJournal, vol.196, p. L71-L75[68] Labeyrie A., "Images of exo-planets obtainable from dark speckles in adaptive optics telescopes"(1995), A&A, vol.298, p544-548[69] Labeyrie A., "Hypertelescope architectures for direct imaging at high angular resolution" (2001),proceeding of "Beyond Conventional Adaptive Optics"[70] Lawson P., "Artefacts in PAPA camera images" (1994), Applied Optics, vol.33, Issue 7, March1, p.1146-1153[71] Lawson P., "The Sydney University PAPA camera" (1994), Astronomical Society of Australia,Proceedings, vol.11, no. 1, p. 50-54[72] Lawson P., "Group-delay tracking in optical stellar interferometry with the fast Fourier transform"(1995), J. Opt. Soc. Am. A, vol.12, p.366[73] Léger A., Mariotti J. M., Mennesson B., Ollivier M., Puget J. L., Rouan, D., Schneider J., "TheDARWIN project" (1996), Astrophysics and Space Science, vol.241, Issue 1, p.135-146[74] Lestrade J.-F., Preston R. A., Jones D. L., Phillips R. B., Rogers A. E. E., Titus M. A., Rioja M.J., Gabuzda D. C., "High-precision VLBI astrometry of radio-emitting stars" (1999), A&A, vol.344,p.1014[75] Lyot B., "La couronne solaire étudiée en dehors des éclipses" (1930), Comptes rendus 191,p.834[76] Lyot B., "Photographie de la couronne solaire en dehors des éclipses" (1931), Comptes rendus193, p.1169[77] Lyot B., "A study of the solar corona and prominences without eclipses" (1939), Monthly Noticeof Royal Academy of Science, vol. 99, p579[78] Mackey C. D., Tubbs R. N., "Sub-Electron Read Noise at MHz Pixel Rates" (2001), SPIE proc.,vol4306, p.289[79] Malbet F., Yu J. W., Shao M., "High-Dynamic-Range Imaging Using a Deformable Mirror for SpaceCoronography" (1995), PASP, vol.107, p.386[80] Malbet F., "High angular resolution coronography for adaptive optics" (1996), A&AS Ser., vol.115,p.161[81] Menesson B., Mariotti J. M., "Array Configurations for a Space Infrared Nulling InterferometerDedicated to the Search for Earthlike Extrasolar Planets" (1997), Icarus, vol.128, p.202-212[82] Mayor M., Queloz D., (1995), nature 378, p.355[83] McAlister H. A., Hartkopf W. I., Hutter D. J., "ICCD speckle observations of binary stars. II. Measurementsduring 1982-1985 from the Kitt Peak 4 m Telescope" (1987), The Astronomical Journal,vol.93, p.688[84] Michel R., Fordham J., Kawamaki H. "Fixed pattern noise in high-resolution, CCD readoutphoton-counting detectors" (1997) Mon. Not. R. Astron. Soc., vol.292, p611-620
Page 1:
Université de Nice-Sophia Antipoli
Page 6 and 7:
Bresson, Jean-Louis Schneider et Je
Page 9:
AbstractThe existence of extra-sola
Page 12 and 13:
3.4 La Coronographie Interférentie
Page 14 and 15:
8.4 Sources de bruit et rapport sig
Page 17:
Introduction1
Page 20 and 21:
4 IntroductionEn guise d’introduc
Page 23 and 24:
Avant ProposJe présente dans cette
Page 25 and 26:
Chapitre 1Point sur la détection d
Page 27 and 28:
Point sur la détection d’exo-pla
Page 29 and 30:
Page 31 and 32:
Page 33 and 34:
Imagerie directe par coronographie
Page 35 and 36:
Chapitre 2Imagerie directe par coro
Page 37 and 38:
Page 39 and 40:
Page 41 and 42:
Page 43 and 44:
Page 45 and 46:
Page 47 and 48:
Page 49 and 50:
Chapitre 3Principes de Coronographi
Page 51 and 52:
Principes de coronographie 35étoil
Page 53 and 54:
Principes de coronographie 37La cor
Page 55 and 56:
Principes de coronographie 39que po
Page 57 and 58:
Chapitre 4Le Coronographe à Coutea
Page 59 and 60:
Coronographie à couteau de phase 4
Page 61 and 62:
Page 63 and 64:
Page 65 and 66:
Page 67 and 68:
Page 69 and 70:
Page 71 and 72:
Page 74 and 75:
58 Coronographie à couteau de phas
Page 76 and 77:
Page 78 and 79:
Page 80 and 81:
64 PKC de laboratoire
Page 82 and 83:
66 PKC de laboratoire5.2 Réalisati
Page 84 and 85:
68 PKC de laboratoirequi se sont av
Page 86 and 87:
70 PKC de laboratoireLa dynamique d
Page 88 and 89:
72 PKC de laboratoire(a)(b)Figure 5
Page 90 and 91:
74 PKC de laboratoireLa Figure 5.9
Page 92 and 93:
76 PKC de laboratoireFigure 5.14. F
Page 94 and 95:
Page 96 and 97:
Page 98 and 99:
Page 100 and 101:
Page 102 and 103:
Page 104 and 105:
88 Caméras à comptage de photons
Page 107 and 108:
Avant ProposDepuis peu, de nouvelle
Page 109 and 110:
Chapitre 6Principes du comptage de
Page 111 and 112:
Principes du comptage de photons 95
Page 113 and 114:
Page 115 and 116:
Page 117 and 118:
Page 119 and 120:
Page 121 and 122:
Chapitre 7Vers une nouvelle archite
Page 123 and 124:
Développement d’une nouvelle arc
Page 125 and 126:
Page 127 and 128:
Page 129 and 130:
Page 131 and 132:
Page 133 and 134:
Page 135 and 136:
Page 137 and 138:
Page 139 and 140:
Page 141 and 142:
Page 143 and 144:
Page 145 and 146:
Page 147 and 148:
Chapitre 8La caméra ALGOLConstruit
Page 149 and 150:
La caméra Algol 133mentation sur l
Page 151 and 152:
La caméra Algol 135paramètres de
Page 153 and 154:
La caméra Algol 1378.2 Couplage in
Page 155 and 156:
La caméra Algol 139T coeur600 nmT
Page 157 and 158:
La caméra Algol 141L’optique de
Page 159 and 160:
La caméra Algol 143Figure 8.10. (g
Page 161 and 162:
La caméra Algol 1458.4.1 Courant d
Page 163 and 164:
La caméra Algol 147Figure 8.13. Ce
Page 165 and 166:
La caméra Algol 149où σ xC est l
Page 167 and 168:
La caméra Algol 151Une troisième
Page 169 and 170:
La caméra Algol 153par seconde), c
Page 171 and 172:
La caméra Algol 1558.10 Cryogénie
Page 173 and 174:
La caméra Algol 157Etoile λ (nm)
Page 175 and 176:
Chapitre 9Exploitation sur le GI2T/
Page 177 and 178:
Exploitation sur GI2T/REGAIN 1619.1
Page 179 and 180:
Exploitation sur GI2T/REGAIN 163Fig
Page 181 and 182:
Exploitation sur GI2T/REGAIN 165qui
Page 183 and 184:
Page 185 and 186:
Page 187 and 188:
Exploitation sur GI2T/REGAIN 171que
Page 189 and 190:
Page 191 and 192:
Exploitation sur GI2T/REGAIN 175Sp
Page 193 and 194:
Page 195 and 196:
Exploitation sur GI2T/REGAIN 179A -
Page 197 and 198:
Exploitation sur GI2T/REGAIN 1811)
Page 199 and 200:
Page 201 and 202: Exploitation sur GI2T/REGAIN 185H,
Page 203 and 204: Exploitation sur GI2T/REGAIN 187qui
Page 205 and 206: Exploitation sur GI2T/REGAIN 189Fic
Page 207 and 208: Exploitation sur GI2T/REGAIN 191
Page 213 and 214: Exploitation sur GI2T/REGAIN 1979.7
Page 215 and 216: Exploitation sur GI2T/REGAIN 1999.8
Page 227: Epilogue211
Page 230 and 231: 214 Epiloguebreux autres thèmes de
Page 233 and 234: Annexe AArticle paru dans A&AS Ser.
Page 235 and 236: Annexe A : publication A&AS Ser. 21
Page 243 and 244: Annexe BProgrammation en parallèle
Page 245 and 246: Annexe B : Programmation en parall
Page 247 and 248: Annexe CListe des nuits d’observa
Page 249 and 250: Bibliographie[1] Abe L., Vakili F.,
Page 251: Bibliographie 235[32] Bruijne (de)
Page 255 and 256: Bibliographie 239[101] Prieur J.-L.
show all

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

You also want an ePaper? Increase the reach of your titles

Delete template?

Save as template?