Volume 514, May 2010
|Number of page(s)||17|
|Section||Celestial mechanics and astrometry|
|Published online||27 May 2010|
Table A.1: Asteroids selected for the individual part of the asteroid model when simultaneously fitting ranging data on all four inner planets. As described in Sect. 6, only asteroids with probability greater than of being removed from the test model during the 100 MC experiments are listed. For each asteroid this probabilty is given together with the asteroid's diameter, density class (in the standard mass set) and correponding perturbations on the Earth-Mars, Earth-Venus, and Earth-Mercury distances in terms of max on the 1969-2010 time interval. Density classes are assigned according to albedo (see Sect. 4.2) and do not always correspond to taxonomies.
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