Czernik 11 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 high 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 (~3.30 kpc) differs significantly from the median photometric distance (~1.78 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	–	39.189	59.637	0.303	-0.606	-0.092	-50.779
Loktin & Popova	2017	39.135	59.632	–	-1.123	-4.417	–
Dias et al.	2014	39.146	59.633	–	-0.08	-0.53	–
Dias et al.	2002	39.146	59.633	–	-0.08	-0.53	–

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