CWNU 4808 is a sparse, very loose object of intermediate 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 intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~15.85 kpc) differs significantly from the median photometric distance (~23.44 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	–	253.619	-49.022	0.063	-3.742	-4.782	-67.041
He et al.	2023	253.631	-49.03	0.077	-3.735	-4.826	–

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