CWNU 4706 is a moderately populated, very loose object of intermediate C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~8.64 kpc) differs significantly from the median photometric distance (~5.75 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	–	105.91	-13.648	0.116	-0.492	1.295	85.156
He et al.	2023	105.899	-13.621	0.106	-0.486	1.307	88.4

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