Dolidze 15 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~3.70 kpc) differs significantly from the median photometric distance (~5.79 kpc).

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	76.664	34.779	0.27	0.767	-1.716	30.345
Bica et al.	2019	76.65	34.859	–	–	–	–
Loktin & Popova	2017	76.65	34.857	–	4.852	-2.251	–
Dias et al.	2014	76.646	34.857	–	1.78	-2.28	–

💡 Note: The UCC values are estimated from its identified members.