| Issue |
A&A
Volume 514, May 2010
|
|
|---|---|---|
| Article Number | A96 | |
| Number of page(s) | 17 | |
| Section | Celestial mechanics and astrometry | |
| DOI | https://doi.org/10.1051/0004-6361/200913346 | |
| Published online | 27 May 2010 | |
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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.