We provide a three-dimensional shape model of near-Earth asteroid (276049) 2002 CE26 based on radar images as reported by Shepard et al. (2006).  The radar data were obtained from Arecibo Observatory and near-infrared spectra from NASA's Infrared Telescope Facility (IRTF) in August and September 2004.  Although the radar data reveal a binary asteroid, and possibly a triple system, only the primary body has a 3-D shape model determined.  The model provides an effective diameter of 3.46 +/- 0.35 km and a synodic rotation period of 3.2931 +/- 0.0003 h.


REFERENCES 
==========
Shepard, M.K., J.L. Margot, C. Magri, M.C. Nolan, J. Schlieder, B. Estes, S.J. Bus, E.L. Volquardsen, A.S. Rivkin, L.A.M. Benner, J.D. Giorgini, S.J. Ostro, M.W. Busch, Radar and infrared observations of binary near-Earth asteroid 2002 CE26, Icarus, 184, 198-210, 2006, doi:10.1016/j.icarus.2006.04.019.