Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..402v&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.402
Computer Science
Scientific paper
The progress in NEA discoveries has led to a situation such that the population of NEAs with H < 16 can be assumed to be complete, or almost complete [3]. This sample of large NEAs is unbiased, and is sufficiently large to allow a meaningful statistical analysis. We compare its statistical features with those of the NEA population model of [1], finding nontrivial differences. In addition, we analyze the evolution of the sample under the action of secular perturbations.
Gronchi Giovanni F.
Valsecchi Giovanni B.
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