FSR 0611 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~5.15 kpc) differs significantly from the median photometric distance (~1.00 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	–	39.373	56.348	0.194	-1.018	0.212	-63.833
Bica et al.	2019	39.42	56.413	–	–	–	–
Dias et al.	2014	39.408	56.415	–	-0.91	-2.28	–
Froebrich et al.	2007	39.408	56.415	–	–	–	–
Dias et al.	2002	39.408	56.415	–	-0.91	-2.28	–

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