X.7. Binary asteroid lightcurves

The Table on p. 5780 – 5787 contains additional data for the lightcurves of the objects marked in the Table “Minor planet lightcurve parameters” as known or suspected binaries. The data are meant to provide a quick overview of a primary period and amplitude of the lightcurves as well as a secondary period and, if available, amplitude. The data for publication in the Table were supplied by B. Warner (Palmer Divide Observatory, Colorado Springs, U.S.A.), A. W. Harris (Space Science Institute, U.S.A.) and P. Pravec (Astronomical Institute, Academy of Sciences of Czech Republic).