SAI 36 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very large^* distance, well 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 (~10.42 kpc) differs significantly from the median photometric distance (~3.00 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	–	64.228	41.091	0.096	-0.229	-0.509	-9.677
Bica et al.	2019	64.208	41.061	–	–	–	–
Glushkova et al.	2010	64.21	41.067	–	–	–	–
Dias et al.	2002	64.208	41.067	–	0.86	-3.77	–

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