Different slices through the phase space of Agg02 (ASCC 19, Gulliver 6, UBC 17a, UBC 17b), together with the complete colour-magnitude diagrams (based on Gaia and 2MASS photometry). Top-left: distribution of parallaxes of all individual stars in Agg02. Duplicates are excluded. Top-right: the histogram of parallaxes, excluding the duplicate cluster members. The best fit was achieved with the following double-Gaussian function parameters: ϖ₁ = 2.364 ± 0.007 mas, σ₁ = 0.134 ± 0.009 mas, ϖ₂ = 2.377 ± 0.008 mas, σ₂ = 0.018 ± 0.011 mas. Middle-left: coordinates of the stars in Agg02. Size of the points indicates values of the observed magnitude G. Middle-right: proper motion diagram of Agg02. Bottom-left: colour-magnitude diagram of Agg02, based on the observed values of B_P − R_P and G). Bottom-right: colour-magnitude diagram of Agg02 based on 2MASS photometry. The stars were located using the coordinates in Gaia database.