Dolidze 14 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~10.43 kpc) differs significantly from the median photometric distance (~1.69 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	–	61.629	27.51	0.096	0.754	-0.92	-13.723
Bica et al.	2019	61.651	27.529	–	–	–	–
Loktin & Popova	2017	61.68	27.543	–	0.151	-6.232	–
Dias et al.	2014	61.679	27.543	–	1.71	-0.88	–
Dias et al.	2002	61.679	27.543	–	1.71	-0.88	–

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