VizieR Online Data Catalog: Photometry and models of long-period asteroids (Marciniak+, 2018)

The files contain asteroid brightness and geometry for corresponding epochs. The "*lcs" files were used for obtaining shape models and spin states of the asteroids using multi-apparition data. Individual lightcurves within a file are separated by an empty line, all lightcurves are relative.

The "*data" files contain the data used for finding the period and contain lightcurves from only one apparition. Here data are relative as well, except for 932 Hooveria and 830 Petropolitana, where all data were calibrated data using CMC15, APASS and GAIA catalogue stars.

(12 data files).