Dolidze 36 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, well above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature, with no articles listed in the last 9 years.

(*): The parallax distance estimate (~5.83 kpc) differs significantly from the median photometric distance (~0.90 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	–	300.58	42.098	0.171	-3.359	-4.088	-37.194
Loktin & Popova	2017	300.54	42.014	–	-0.93	-4.477	77.0
Dias et al.	2014	300.625	42.1	–	-1.47	-3.39	77.0
Piskunov et al.	2008	300.591	42.151	–	–	–	–
Kharchenko et al.	2005	300.6	42.15	–	0.19	-0.95	–
Dias et al.	2002	300.625	42.1	–	-1.47	-3.39	77.0

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