CWNU 4760 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~8.35 kpc) differs significantly from the median photometric distance (~5.50 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	–	105.042	-15.332	0.12	-0.395	1.207	123.222
He et al.	2023	105.032	-15.357	0.119	-0.388	1.187	73.0

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