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

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234 Bibliographie[14] Baldwin J. E., Tubbs R. N., Cox G. C., Mackay C. D., Wilson R. W., Andersen, M. I., "Diffractionlimitted800nm imaging with the 2.56m Nordic Optical Telescope" 2001, A&A, vol.368, p.L1[15] Barth W., Weigelt G., Zinnecker H., "Speckle masking observations of the young binary Z CanisMajoris" (1994), vol.291, no. 2, p. 500-504[16] Baudoz P., "Coronographie Stellaire : Le Coronographe Interférentiel Achromatique" (1999),Thèse de Doctorat, Université de Nice Sophia-Antipolis[17] Baudoz P., "Achromatic interfero coronagraphy. II. Effective performance on the sky" (2000),A&AS Ser., vol.145, p.341[18] Beckers J. M., "Detailed compensation of atmospheric seeing using multiconjugate adaptive optics"(1989), Proc. SPIE vol.1114, p.215[19] Bergamini P., Bonelli G., Poletto L., Tanzi E.G., Tondello G., Uslenghi M. "Characterization ofa Photon-Counting ICCD Prototype" (1998), SPIE[20] Berio P., Vakili, F., Mourard, D. and Bonneau, D., "Removing the photon-centroiding hole inoptical stellar interferometry" (1998), A&AS Ser., vol.129, p609-615[21] Berio P., Mourard D., Bonneau D., Chesneau O., Stee P., Thureau N., Vakili F. & Borgnino J.,"Spectrally resolved Michelson Interferometry. I. Exact formalism in the multi-speckle mode" (1999),J. Opt. Soc. Am., vol.16, p872[22] Biesecker D. A., Lamy P., St. Cyr O. C., Llebaria A., & Howard R. A., "Sungrazing CometsDiscovered with the SOHO/LASCO Coronagraphs 1996-1998" (2002), Icarus, vol.157, p.323[23] Blazit A. (1988), Thèse d’Etat[24] Boccaletti A., Labeyrie A. and Ragazzoni R., "Prelimiray results of dark-speckles stellar coronagraphy"(1998), A&A, vol.338, p106-110[25] Boccaletti A., Moutou C., Labeyrie A., Kohler D., Vakili F., "Present performance of the darkspecklecoronagraph" (1998), A&AS Ser.[26] Boccaletti A., Moutou C., Abe L., "Refined laboratory simulations of dark-speckle coronagraphy"(1999) A&AS, vol.141, p.157-164[27] Boccaletti A., Moutou C., Abe L., Vakili F., Labeyrie A., Riaud P., Schneider J., "NEF : NGSTExo-planet Finder : I. Concepts" (2000), Proceedings of the Next Generation Space TelescopeScience and Technology, ASP Conference Series, vol.207, p.179[28] Boccaletti A., Moutou C., Mouillet D., Lagrange A.-M., Augereau J.-C., "Dark-speckle coronagraphicdetection of binary stars in the near-IR" (2001), A&A, vol.367, p.371[29] Bonneau D., Josse M. and Labeyrie A., "Lock-in image subtraction : detectability of circumstellarplanets with the large space telescope" (1975), Image Processing Techniques in Astronomy, p.403-409[30] Bourget P., Veiga C. H., Vieira Martins R. "A Coronagraph with a Variable-Diameter OccultingDisk" (2001), PASP, vol.113, p.436-438[31] Bracewell, R. B., "Detecting nonsolar planets by spinning infrared interferometer" (1978), Nature,274, 780
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Université de Nice-Sophia Antipoli
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Bresson, Jean-Louis Schneider et Je
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AbstractThe existence of extra-sola
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3.4 La Coronographie Interférentie
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8.4 Sources de bruit et rapport sig
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Introduction1
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4 IntroductionEn guise d’introduc
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Avant ProposJe présente dans cette
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Chapitre 1Point sur la détection d
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Point sur la détection d’exo-pla
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Imagerie directe par coronographie
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Chapitre 2Imagerie directe par coro
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Chapitre 3Principes de Coronographi
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Principes de coronographie 35étoil
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Principes de coronographie 37La cor
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Principes de coronographie 39que po
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Chapitre 4Le Coronographe à Coutea
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Coronographie à couteau de phase 4
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58 Coronographie à couteau de phas
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64 PKC de laboratoire
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66 PKC de laboratoire5.2 Réalisati
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68 PKC de laboratoirequi se sont av
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70 PKC de laboratoireLa dynamique d
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72 PKC de laboratoire(a)(b)Figure 5
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74 PKC de laboratoireLa Figure 5.9
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76 PKC de laboratoireFigure 5.14. F
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88 Caméras à comptage de photons
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Avant ProposDepuis peu, de nouvelle
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Chapitre 6Principes du comptage de
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Principes du comptage de photons 95
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Chapitre 7Vers une nouvelle archite
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Développement d’une nouvelle arc
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Chapitre 8La caméra ALGOLConstruit
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La caméra Algol 133mentation sur l
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La caméra Algol 135paramètres de
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La caméra Algol 1378.2 Couplage in
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La caméra Algol 139T coeur600 nmT
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La caméra Algol 141L’optique de
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La caméra Algol 143Figure 8.10. (g
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La caméra Algol 1458.4.1 Courant d
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La caméra Algol 147Figure 8.13. Ce
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La caméra Algol 149où σ xC est l
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La caméra Algol 151Une troisième
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La caméra Algol 153par seconde), c
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La caméra Algol 1558.10 Cryogénie
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La caméra Algol 157Etoile λ (nm)
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Chapitre 9Exploitation sur le GI2T/
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Exploitation sur GI2T/REGAIN 1619.1
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Exploitation sur GI2T/REGAIN 163Fig
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Exploitation sur GI2T/REGAIN 165qui
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Exploitation sur GI2T/REGAIN 171que
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Exploitation sur GI2T/REGAIN 175Sp
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Exploitation sur GI2T/REGAIN 179A -
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Exploitation sur GI2T/REGAIN 1811)
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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: Bibliographie[1] Abe L., Vakili F.,
Page 253 and 254: Bibliographie 237[67] Labeyrie A.,
Page 255 and 256: Bibliographie 239[101] Prieur J.-L.
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