Techniques d'observation spectroscopique d'astÃ©roÃ¯des

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tel-00785991, version 1 - 7 Feb 2013 10 M. Birlan et al. Birlan M., Barucci M. A., Vernazza P., Fulchignoni M., Binzel R. P., Bus S. J., Belskaya I., Fornasier S., 2004, New Astronomy, 9, 343 Birlan M., Vernazza P., Fulchignoni M., Barucci M. A., Descamps P., Binzel R. P., Bus S. J., 2006, A&A, 454, 677 Burbine T. H., Buchanan P. C., Dolkar T., Binzel R. P., 2009, Meteoritics and Planetary Science, 44, 1331 Canas L., Duffard R., Seixas T., 2008, Earth Moon and Planets, 102, 543 Cellino A., Pannunzio R., Zappala V., Farinella P., Paolicchi P., 1985, A&A, 144, 355 Cloutis E. A., Gaffey M. J., 1991a, J. Geophys. Res., 96, 22809 Cloutis E. A., Gaffey M. J., 1991b, Earth Moon and Planets, 53, 11 Cushing M. C., Vacca W. D., Rayner J. T., 2004, Planet. Space Sci., 116, 362 Dell’Oro A., Cellino A., 2007, MNRAS, 380, 399 DeMeo F. E., Binzel R. P., Slivan S. M., Bus S. 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Vernazza P., Mothé-Diniz T., Barucci M. A., Birlan M., Carvano J. M., Strazzulla G., Fulchignoni M., Migliorini A., 2005, A&A, 436, 1113 Warner B. D., 2002, Minor Planet Bulletin, 29, 74 Wijesinghe M. P., Tedesco E. F., 1979, Icarus, 40, 383 Zappala V., Bendjoya P., Cellino A., Farinella P., Froeschle C., 1995, Icarus, 116, 291 Zappala V., Scaltriti F., Farinella P., Paolicchi P., 1980, Moon and Planets, 22, 153 Spectral properties of (854), (1333), and (3623) 11 tel-00785991, version 1 - 7 Feb 2013 c○ 0000 RAS, MNRAS 000, 000–000
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OBSERVATOIRE DE PARIS ÉCOLE DOCTOR
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tel-00785991, version 1 - 7 Feb 201
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Résumé: L’objectif fondamental
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Acknowledgements tel-00785991, vers
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Dedicated to mygrandfather, IosifPo
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Contents Tables 22 Figures 27 I INT
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7.4.2 (3623) Chaplin . . . . . . .
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List of Tables 2.1 The emission lin
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List of Figures 1.1 A field obtaine
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5.8 Asteroid spectra and the best t
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1 Why asteroids? tel-00785991, vers
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CHAPTER 1. WHY ASTEROIDS? 33 tel-00
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CHAPTER 1. WHY ASTEROIDS? 39 the fi
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2 Why spectroscopy? spectrum. By ca
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CHAPTER 2. WHY SPECTROSCOPY? 45 0.4
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CHAPTER 2. WHY SPECTROSCOPY? 47 The
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CHAPTER 2. WHY SPECTROSCOPY? 49 0.6
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CHAPTER 2. WHY SPECTROSCOPY? 51 −
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CHAPTER 2. WHY SPECTROSCOPY? 53 tel
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3 Observing techniques tel-00785991
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CHAPTER 3. OBSERVING TECHNIQUES 59
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4 Spectral analysis techniques tel-
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CHAPTER 4. SPECTRAL ANALYSIS TECHNI
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5 M4AST - Modeling of Asteroids Spe
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CHAPTER 5. M4AST - MODELING OF ASTE
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6 Spectral properties of near-Earth
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CHAPTER 6. SPECTRAL PROPERTIES OF N
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7 Spectral properties of Main Belt
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CHAPTER 7. SPECTRAL PROPERTIES OF M
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8 Conclusions and perspectives tel-
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A The GuideDog and the BigDog inter
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B List of publications B.1 First Au
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APPENDIX B. LIST OF PUBLICATIONS 13
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Bibliography Adams, J. B. 1974. Vis
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BIBLIOGRAPHY 143 Brunetto, R., Vern
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BIBLIOGRAPHY 145 Donnison, J. R. 19
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