150 BIBLIOGRAPHY tel-00785991, version 1 - 7 Feb 2013 Storrs, A., Weiss, B., Zellner, B., Burleson, W., Sichitiu, R., Wells, E., Kowal, C., & Tholen, D. 1999. Imaging Observations of Asteroids with Hubble Space Telescope. Icarus, 137(Feb.), 260–268. Stuart, J. S., & Binzel, R. P. 2004. Bias-corrected population, size distribution, and impact hazard for the near-Earth objects. Icarus, 170(Aug.), 295–311. Sunshine, J. M., & Pieters, C. M. 1993. Estimating modal abundances from the spectra of natural and laboratory pyroxene mixtures using the modified Gaussian model. J. Geophys. Res., 98(May), 9075–9087. Sunshine, J. M., & Pieters, C. M. 1998. Determining the composition of olivine from reflectance spectroscopy. J. Geophys. Res., 103(June), 13675–13688. Sunshine, J. M., Bus, S. J., Corrigan, C. M., McCoy, T. J., & Burbine, T. H. 2007. Olivinedominated asteroids and meteorites: Distinguishing nebular and igneous histories. Meteoritics and planetary science, 42(Aug.), 155–170. Taylor, P. A., Howell, E. S., Magri, C., Vervack, R. J., Nolan, M. C., Fernandez, Y. R., Rivkin, A. S., & Mueller, M. 2009 (Sept.). Variability of Thermal Infrared Emission from Near- Earth Asteroids. Pages 32.01–+ of: Aas/division for planetary sciences meeting abstracts. AAS/Division for Planetary Sciences Meeting Abstracts, vol. 41. Tedesco, E. F. 1979. Binary asteroids - Evidence for their existence from lightcurves. Science, vol. 203, mar. 2, 1979, p. 905-907., 203(Mar.), 905–907. Tennyson, J. 2005. Astronomical spectroscopy : an introduction to the atomic and molecular physics of astronomical spectra. Tholen, D. J. 1984 (Sept.). Asteroid taxonomy from cluster analysis of Photometry. Ph.D. thesis, Arizona Univ., Tucson. Thomas, P. C., Binzel, R. P., Gaffey, M. J., Zellner, B. H., Storrs, A. D., & Wells, E. 1997. Vesta: Spin Pole, Size, and Shape from HST Images. Icarus, 128(July), 88–94. Tonry, J., & Davis, M. 1979. A survey of galaxy redshifts. I - Data reduction techniques. AJ, 84(Oct.), 1511–1525. Trevese, D., Paris, D., Stirpe, G. M., Vagnetti, F., & Zitelli, V. 2007. Line and continuum variability of two intermediate-redshift, high-luminosity quasars. A&A, 470(Aug.), 491–496. Vacca, W. D., Cushing, M. C., & Rayner, J. T. 2004. Nonlinearity Corrections and Statistical Uncertainties Associated with Near-Infrared Arrays. PASP, 116(Apr.), 352–361. Vaduvescu, O., Popescu, M., Comsa, I, & et. all. 2012. Mining the ESO WFI and INT WFC archives for known Near Earth Asteroids. Mega-Precovery Software. Astronomische nachrichten (astronomical notes), In press. van Flandern, T. C., Tedesco, E. F., & Binzel, R. P. 1979. Satellites of asteroids. Pages 443–465. Vander Haagen, G. A. 2011. Lightcurve for Near-Earth Asteroid (164400) 2005 GN59. Minor planet bulletin, 38(Jan.), 10–11. Vernazza, P.. 2006. Etude des Proprietes Physiques des Asteroides. Ph.D. thesis, Observatoire de Paris.
BIBLIOGRAPHY 151 tel-00785991, version 1 - 7 Feb 2013 Vernazza, P., Binzel, R. P., DeMeo, F. E., & Thomas, C. A. 2007 (Oct.). Mineralogical Characterization Of 150 S-type Asteroids And Comparison With OC Meteorites. Page 476 of: Aas/division for planetary sciences meeting abstracts #39. Bulletin of the American Astronomical Society, vol. 38. Vernazza, P., Binzel, R. P., Thomas, C. A., DeMeo, F. E., Bus, S. J., Rivkin, A. S., & Tokunaga, A. T. 2008. Compositional differences between meteorites and near-Earth asteroids. Nature, 454(Aug.), 858–860. Vernazza, P., Binzel, R. P., Rossi, A., Fulchignoni, M., & Birlan, M. 2009. Solar wind as the origin of rapid reddening of asteroid surfaces. Nature, 458(Apr.), 993–995. Veverka, J., Robinson, M., Thomas, P., Murchie, S., Bell, J. F., Izenberg, N., Chapman, C., Harch, A., Bell, M., Carcich, B., Cheng, A., Clark, B., Domingue, D., Dunham, D., Farquhar, R., Gaffey, M. J., Hawkins, E., Joseph, J., Kirk, R., Li, H., Lucey, P., Malin, M., Martin, P., McFadden, L., Merline, W. J., Miller, J. K., Owen, W. M., Peterson, C., Prockter, L., Warren, J., Wellnitz, D., Williams, B. G., & Yeomans, D. K. 2000. NEAR at Eros: Imaging and Spectral Results. Science, 289(Sept.), 2088–2097. Vokrouhlický, D., & Nesvorný, D. 2008. Pairs of Asteroids Probably of a Common Origin. AJ, 136(July), 280–290. Walsh, K. J., Delbo’, M., Mueller, M., Binzel, R. P., & DeMeo, F. E. 2012. Physical Characterization and Origin of Binary Near-Earth Asteroid (175706) 1996 FG 3 . ApJ, 748(Apr.), 104. Warner, B. D. 2002. Asteroid Photometry at the Palmer Divide Observatory: Results for 1333 Cevenola and 2460 Mitlincoln. The minor planet bulletin, volume 29, p.74-75, 29(Dec.), 74–75. Warner, B. D. 2009. Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 May - September. Minor planet bulletin, 36(Jan.), 7–13. West, J. L., & Cameron, I. D. 2006. Using the Medical Image-Processing Package, ImageJ, for Astronomy. JRASC, 100(Dec.), 242. Wijesinghe, M. P., & Tedesco, E. F. 1979. A test of plausibility of eclipsing binary asteroids. Icarus, 40(Dec.), 383–393. Wisniewski, W. Z., Michalowski, T. M., Harris, A. W., & McMillan, R. S. 1997. Photometric Observations of 125 Asteroids. Icarus, 126(Apr.), 395–449. Wolters, S. D., Rozitis, B., Duddy, S. R., Lowry, S. C., Green, S. F., Snodgrass, C., Hainaut, O. R., & Weissman, P. 2011. Physical characterization of low delta-V asteroid (175706) 1996 FG3. MNRAS, 418(Dec.), 1246–1257. Xu, S., Binzel, R. P., Burbine, T. H., & Bus, S. J. 1995. Small main-belt asteroid spectroscopic survey: Initial results. Icarus, 115(May), 1–35. Yamada, M., Sasaki, S., Fujiwara, A., Hiroi, T., Hasegawa, S., Nagahara, H., Ohashi, H., Ohtake, H., & Yano, H. 1999 (Mar.). Simulation of Space Weathering by Nanosecond Pulse Laser Heating and Proton Implantation: Difference of Olivine and Pyroxene Samples. Page 1566 of: Lunar and planetary institute science conference abstracts. Lunar and Planetary Institute Science Conference Abstracts, vol. 30.
- Page 1 and 2:
OBSERVATOIRE DE PARIS ÉCOLE DOCTOR
- Page 3 and 4:
OBSERVATOIRE DE PARIS ÉCOLE DOCTOR
- Page 5 and 6:
OBSERVATOIRE DE PARIS ÉCOLE DOCTOR
- Page 7 and 8:
tel-00785991, version 1 - 7 Feb 201
- Page 9 and 10:
Résumé: L’objectif fondamental
- Page 11 and 12:
tel-00785991, version 1 - 7 Feb 201
- Page 13 and 14:
Acknowledgements tel-00785991, vers
- Page 15 and 16:
Dedicated to mygrandfather, IosifPo
- Page 17 and 18:
Contents Tables 22 Figures 27 I INT
- Page 19 and 20:
7.4.2 (3623) Chaplin . . . . . . .
- Page 21 and 22:
List of Tables 2.1 The emission lin
- Page 23 and 24:
List of Figures 1.1 A field obtaine
- Page 25 and 26:
5.8 Asteroid spectra and the best t
- Page 27 and 28:
tel-00785991, version 1 - 7 Feb 201
- Page 29 and 30:
tel-00785991, version 1 - 7 Feb 201
- Page 31 and 32:
1 Why asteroids? tel-00785991, vers
- Page 33 and 34:
CHAPTER 1. WHY ASTEROIDS? 33 tel-00
- Page 35 and 36:
CHAPTER 1. WHY ASTEROIDS? 35 tel-00
- Page 37 and 38:
CHAPTER 1. WHY ASTEROIDS? 37 tel-00
- Page 39 and 40:
CHAPTER 1. WHY ASTEROIDS? 39 the fi
- Page 41 and 42:
tel-00785991, version 1 - 7 Feb 201
- Page 43 and 44:
2 Why spectroscopy? spectrum. By ca
- Page 45 and 46:
CHAPTER 2. WHY SPECTROSCOPY? 45 0.4
- Page 47 and 48:
CHAPTER 2. WHY SPECTROSCOPY? 47 The
- Page 49 and 50:
CHAPTER 2. WHY SPECTROSCOPY? 49 0.6
- Page 51 and 52:
CHAPTER 2. WHY SPECTROSCOPY? 51 −
- Page 53 and 54:
CHAPTER 2. WHY SPECTROSCOPY? 53 tel
- Page 55 and 56:
tel-00785991, version 1 - 7 Feb 201
- Page 57 and 58:
3 Observing techniques tel-00785991
- Page 59 and 60:
CHAPTER 3. OBSERVING TECHNIQUES 59
- Page 61 and 62:
CHAPTER 3. OBSERVING TECHNIQUES 61
- Page 63 and 64:
CHAPTER 3. OBSERVING TECHNIQUES 63
- Page 65 and 66:
4 Spectral analysis techniques tel-
- Page 67 and 68:
CHAPTER 4. SPECTRAL ANALYSIS TECHNI
- Page 69 and 70:
CHAPTER 4. SPECTRAL ANALYSIS TECHNI
- Page 71 and 72:
CHAPTER 4. SPECTRAL ANALYSIS TECHNI
- Page 73 and 74:
CHAPTER 4. SPECTRAL ANALYSIS TECHNI
- Page 75 and 76:
CHAPTER 4. SPECTRAL ANALYSIS TECHNI
- Page 77 and 78:
5 M4AST - Modeling of Asteroids Spe
- Page 79 and 80:
CHAPTER 5. M4AST - MODELING OF ASTE
- Page 81 and 82:
CHAPTER 5. M4AST - MODELING OF ASTE
- Page 83 and 84:
CHAPTER 5. M4AST - MODELING OF ASTE
- Page 85 and 86:
CHAPTER 5. M4AST - MODELING OF ASTE
- Page 87 and 88:
CHAPTER 5. M4AST - MODELING OF ASTE
- Page 89 and 90:
CHAPTER 5. M4AST - MODELING OF ASTE
- Page 91 and 92:
tel-00785991, version 1 - 7 Feb 201
- Page 93 and 94:
6 Spectral properties of near-Earth
- Page 95 and 96:
CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 97 and 98:
CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 99 and 100: CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 101 and 102: CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 103 and 104: CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 105 and 106: CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 107 and 108: CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 109 and 110: CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 111 and 112: CHAPTER 6. SPECTRAL PROPERTIES OF N
- Page 113 and 114: 7 Spectral properties of Main Belt
- Page 115 and 116: CHAPTER 7. SPECTRAL PROPERTIES OF M
- Page 117 and 118: CHAPTER 7. SPECTRAL PROPERTIES OF M
- Page 119 and 120: CHAPTER 7. SPECTRAL PROPERTIES OF M
- Page 121 and 122: CHAPTER 7. SPECTRAL PROPERTIES OF M
- Page 123 and 124: CHAPTER 7. SPECTRAL PROPERTIES OF M
- Page 125 and 126: CHAPTER 7. SPECTRAL PROPERTIES OF M
- Page 127 and 128: CHAPTER 7. SPECTRAL PROPERTIES OF M
- Page 129 and 130: CHAPTER 7. SPECTRAL PROPERTIES OF M
- Page 131 and 132: tel-00785991, version 1 - 7 Feb 201
- Page 133 and 134: 8 Conclusions and perspectives tel-
- Page 135 and 136: A The GuideDog and the BigDog inter
- Page 137 and 138: B List of publications B.1 First Au
- Page 139 and 140: APPENDIX B. LIST OF PUBLICATIONS 13
- Page 141 and 142: Bibliography Adams, J. B. 1974. Vis
- Page 143 and 144: BIBLIOGRAPHY 143 Brunetto, R., Vern
- Page 145 and 146: BIBLIOGRAPHY 145 Donnison, J. R. 19
- Page 147 and 148: BIBLIOGRAPHY 147 tel-00785991, vers
- Page 149: BIBLIOGRAPHY 149 Popescu, M., Birla
- Page 153 and 154: tel-00785991, version 1 - 7 Feb 201
- Page 155 and 156: A&A 535, A15 (2011) Table 1. Log of
- Page 157 and 158: A&A 535, A15 (2011) tel-00785991, v
- Page 159 and 160: A&A 535, A15 (2011) Table 3. Summar
- Page 161 and 162: A&A 535, A15 (2011) tel-00785991, v
- Page 163 and 164: Band I center [um] 1.04 1.02 1 0.98
- Page 165 and 166: A&A 544, A130 (2012) DOI: 10.1051/0
- Page 167 and 168: M. Popescu et al.: M4AST - Modeling
- Page 169 and 170: M. Popescu et al.: M4AST - Modeling
- Page 171 and 172: M. Popescu et al.: M4AST - Modeling
- Page 173 and 174: M. Popescu et al.: M4AST - Modeling
- Page 175 and 176: U.P.B. Sci. Bull., Series A, Vol. 7
- Page 177 and 178: Applications of optical and infrare
- Page 179 and 180: Applications of optical and infrare
- Page 181 and 182: Applications of optical and infrare
- Page 183 and 184: Applications of optical and infrare
- Page 185 and 186: Applications of optical and infrare
- Page 187 and 188: Applications of optical and infrare
- Page 189 and 190: Mon. Not. R. Astron. Soc. 000, 000-
- Page 191 and 192: Spectral properties of (854), (1333
- Page 193 and 194: Spectral properties of (854), (1333
- Page 195 and 196: Spectral properties of (854), (1333
- Page 197 and 198: Spectral properties of (854), (1333
- Page 199: Vernazza P., Mothé-Diniz T., Baruc