Comparison between distances and extinctions obtained in this paper with those obtained by Bossini et al. (2019), but in this case for the same input photometry as StarHorse and with PARSEC models, for open clusters. Each panel corresponds to an open cluster with more than ten member candidates observed by APOGEE. The median StarHorse results for individual stars in each cluster are shown as red crosses (dwarfs) and blue open circles (giants). The horizontal and vertical lines correspond to the median values and 1σ limits inferred by Bossini et al. (2019) through isochrone fitting.