Broad-band Photometric Monitoring of 1226 Golia and 6349 Acapulco

Broad-band photometric monitoring of 1226 Golia and 6349 Acapulco was carried out in 2021 February-March. For 1226 Golia, we report a rotation period of 4.46 ± 0.05 h and a V-band variability amplitude of 0.41 ± 0.02 mag, which are in agreement with the range of previously reported measurements. For 6349 Acapulco, we find typical colors for a C-type asteroid of B-V = 0.7 ± 0.1 mag and V-R = 0.3 ± 0.1 mag and little evidence for color changes as a function of time. We report a rotation period of 4.48 ± 0.05 h that is in good agreement with a previous measurement, and a variability amplitude of 0.55 ± 0.02 mag that is three times larger than previously reported.