Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes

[1]  D. Koschny,et al.  Relevance of asteroid occultation measurements to determination of characteristics of near-Earth objects , 2010 .

[2]  S. Ostro,et al.  Radar imaging of Asteroid 7 Iris , 2010 .

[3]  Mikko Kaasalainen,et al.  DAMIT: a database of asteroid models , 2010 .

[4]  Thierry Fusco,et al.  Physical Properties of (2) Pallas , 2009, 0912.3626.

[5]  Christopher T. Russell,et al.  The Shape and Surface Variation of 2 Pallas from the Hubble Space Telescope , 2009, Science.

[6]  J. C. Clark,et al.  A Trio of Well-Observed Asteroid Occultations in 2008 , 2009 .

[7]  Petr Pravec,et al.  The asteroid lightcurve database , 2009 .

[8]  S. Degenhardt.  High Resolution Asteroid Profile by Multi Chord Occultation Observations , 2009 .

[9]  J. Michałowski,et al.  Photometry and models of selected main belt asteroids. VI. 160 Una, 747 Winchester, and 849 Ara , 2009 .

[10]  Paolo Tanga,et al.  Thermal inertia of main belt asteroids smaller than 100 km from IRAS data , 2008, 0808.0869.

[11]  Brian Warner,et al.  Asteroid models from combined sparse and dense photometric data , 2009 .

[12]  F. Marchis,et al.  2007 Mutual events within the binary system of (22) Kalliope , 2008 .

[13]  B. Warner,et al.  Shape and Spin Models for Four Asteroids , 2008 .

[14]  P. Tanga,et al.  Asteroid occultations today and tomorrow: toward the GAIA era , 2007, 0801.2684.

[15]  T. Hayamizu,et al.  Occultation by (22) Kalliope and its satellite Linus , 2007, Proceedings of the International Astronomical Union.

[16]  R. Roy,et al.  Photometry and models of selected main belt asteroids - IV. 184 Dejopeja, 276 Adelheid, 556 Phyllis , 2007 .

[17]  Giovanni B. Valsecchi,et al.  Near earth objects, our celestial neighbors : opportunity and risk : proceedings of the 236th Symposium of the International Astronomical Union held in Prague, Czech Republic, August 14-18, 2006 , 2007 .

[18]  B. Thompson,et al.  Duplicity in 16 Piscium Confirmed from Its Occultation by 7 Iris on 2006 May 5 , 2006 .

[19]  M. Kaasalainen,et al.  Photometry and models of selected main belt asteroids. III. 283 Emma, 665 Sabine, and 690 Wratislavia , 2006 .

[20]  J Berthier,et al.  Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey. , 2006, Icarus.

[21]  E. F. Tedesco,et al.  Asteroid albedos deduced from stellar occultations , 2006 .

[22]  D. Dunham.  Upcoming Asteroid Occultations , 2006 .

[23]  T. Grav,et al.  Physical models of asteroids from sparse photometric data , 2006, Proceedings of the International Astronomical Union.

[24]  Sanna Kaasalainen,et al.  Ground reference for space remote sensing. Laboratory photometry of an asteroid model , 2005 .

[25]  D. Dunham.  Asteroid Occultations for March-July 2005 , 2005 .

[26]  D. Dunham.  Celestial calendar: asteroid occultations for March-July 2005 , 2005 .

[27]  Stephen D. Price,et al.  IRAS Minor Planet Survey V6.0 , 2004 .

[28]  M. Kaasalainen,et al.  Photometry and models of selected main belt asteroids I. 52 Europa, 115 Thyra, and 382 Dodona , 2004 .

[29]  Mikko Kaasalainen,et al.  Shapes and rotational properties of thirty asteroids from photometric data , 2003 .

[30]  M. Kaasalainen,et al.  Photometric signatures of highly nonconvex and binary asteroids , 2003 .

[31]  M. Lattanzi,et al.  Asteroid observations with the Hubble Space Telescope FGS - II. Duplicity search and size measurements for 6 asteroids , 2003 .

[32]  Richard P. Binzel,et al.  Spin vectors in the Koronis family: comprehensive results from two independent analyses of 213 rotation lightcurves , 2003 .

[33]  M. Kaasalainen,et al.  Models of Twenty Asteroids from Photometric Data , 2002 .

[34]  M. Kaasalainen,et al.  Binary structures among large asteroids , 2002 .

[35]  D. Dunham.  Planetary occultations for 2002 , 2002 .

[36]  Karri Muinonen,et al.  Optimization Methods for Asteroid Lightcurve Inversion. II. The Complete Inverse Problem , 2001 .

[37]  M. Kaasalainen,et al.  Optimization Methods for Asteroid Lightcurve Inversion: I. Shape Determination , 2001 .

[38]  H. Fukushima,et al.  Size and Shape of Trojan Asteroid Diomedes from Its Occultation and Photometry , 2000 .

[39]  P. Murdin.  Uppsala Astronomical Observatory , 2000 .

[40]  M. Kaasalainen,et al.  Optimization methods for asteroid lightcurve inversion , 1999 .

[41]  D. Dunham.  Planetary Occultations for 1998 , 1998 .

[42]  T. P. Ojha,et al.  Physical Properties of Soybean , 1993 .

[43]  M. Sộma,et al.  The Occultation of Gamma Geminorum by the Asteroid 381 Myrrha , 1993 .

[44]  R. Binzel,et al.  The size and shape of (2) Pallas from the 1983 occultation of 1 Vulpeculae , 1990 .

[45]  W. J. Cocke,et al.  Triaxial ellipsoid dimensions and rotational pole of 2 Pallas from two stellar occultations , 1989 .

[46]  J. Piironen,et al.  Asteroid photometric catalogue : first update , 1988 .

[47]  J. Stamm.  Reports of asteroidal appulses and occultations. , 1987 .

[48]  E. Tedesco,et al.  M-class Asteroids among the Near-Earth Asteroid Population , 1986 .

[49]  J. Stamm.  Asteroidal appulse and occultation observations. , 1985 .

[50]  P. M. Price,et al.  The diameter of 88 Thisbe from its occultation of SAO 187124 , 1983 .

[51]  N. White,et al.  The diameter of Juno from its occultation of AG + 0 deg 1022 , 1981 .

[52]  N. White,et al.  The diameter of Pallas from its occultation of SAO 85009 , 1979 .

[53]  R. Millis,et al.  Direct determination of asteroid diameters from occultation observations , 1979 .

[54]  G. E. Taylor,et al.  The size of minor planet 6 Hebe , 1978 .