CWNU 3075 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~29.76 kpc) differs significantly from the median photometric distance (~11.48 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	–	299.495	36.046	0.034	-1.75	-2.592	-146.571
He et al.	2023	299.492	36.05	0.042	-1.75	-2.55	-146.57

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