Online Material
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.