CWNU 4807 is a sparse, 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 intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~18.80 kpc) differs significantly from the median photometric distance (~10.00 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	–	295.769	28.659	0.053	-2.22	-4.226	-78.127
He et al.	2023	295.77	28.674	0.064	-2.206	-4.238	–

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