%R 2010PDSS..118G
%A Gladman, B.J.;Davis, D.R.;Neese, C.;Jedicke, R.;Williams, G.;Kavelaars, J.J.;Petit, J-M.;Scholl, H.;Holman, M.;Warrington, B.;Esquerdo, G.;Tricarico, P.
%T Sub-Kilometer Asteroid Diameter Survey (SKADS) V1.0
%D 05/2010
%J NASA Planetary Data System, EAR-A-I0655-5-SKADS-V1.0
%U http://pdsquery.jpl.nasa.gov/query?Identifier=EAR-A-I0655-5-SKADS-V1.0&resclass=data.dataset
%B The Sub-Kilometer Asteroid Diameter Survey (SKADS) (Gladman et al. 2009) acquired good-quality orbital and absolute magnitude (H) determinations for a sample of small main-belt asteroids in order to study the orbital and size distribution beyond H = 15, down to sub-kilometer sizes (H > 18).  Based on six observing nights over an 11-night baseline, SKADS detected, measured photometry for, and linked observations of 1087 asteroids which have one-week time baselines or more.  This data set contains the astrometry, photometry, and orbits of the 1087 asteroids detected by SKADS.