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Fig. 1.

image

Different slices through the phase space of Agg07 (Alessi 5, BH 99), together with the complete colour-magnitude diagrams (based on Gaia and 2MASS photometry). Top: histogram of parallaxes, excluding the duplicate cluster members. The best fit was achieved with the following double-Gaussian function parameters: ϖ1 = 2.225 ± 0.007 mas, σ1 = 0.087 ± 0.007 mas, ϖ2 = 2.501 ± 0.006 mas, σ2 = 0.061 ± 0.006 mas. Middle-left: coordinates of the stars in Agg07. Size of the points indicates values of the observed magnitude G. Middle-right: proper motion diagram of Agg07. Bottom-left: colour-magnitude diagram based on the observed values of BP − RP and G). Bottom-right: colour-magnitude diagram based on 2MASS photometry. The stars were located using the coordinates in Gaia database. The two clusters remain distinguishable in this photometric system.

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