Comparison of the kinematic distances of YSOs in the IRAS 22147 region obtained using CO observations and the distances from Gaia (Bailer-Jones et al. 2021). Black empty squares show the kinematic distance obtained using CO emission (Section 3.1). Blue dots, green crosses, and red dots show the 14th, 50th (median), and the 86th percentile of photogeometric distance distribution. The full names of YSOs and their equatorial coordinates are provided in Table A.1.