FSR 1204 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~4.16 kpc) differs significantly from the median photometric distance (~1.71 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	–	107.113	-12.92	0.24	-0.629	1.26	54.869
Bica et al.	2019	107.084	-12.896	–	–	–	–
Froebrich et al.	2007	107.083	-12.891	–	–	–	–
Dias et al.	2002	107.083	-12.891	–	-2.58	2.95	–

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