Dolidze 24 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 9 years.

(*): The parallax distance estimate (~4.69 kpc) differs significantly from the median photometric distance (~2.56 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	–	101.188	1.731	0.213	-0.705	0.259	106.65
Loktin & Popova	2017	101.175	1.686	–	-0.273	-0.967	–
Dias et al.	2014	101.171	1.685	–	-0.57	-1.24	–
Dias et al.	2002	101.171	1.685	–	-0.57	-1.24	–

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