FSR 0733 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~5.16 kpc) differs significantly from the median photometric distance (~1.50 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	–	71.26	39.758	0.194	0.565	0.095	-10.619
Bica et al.	2019	71.288	39.771	–	–	–	–
Dias et al.	2014	71.283	39.776	–	1.46	-4.38	–
Froebrich et al.	2007	71.283	39.776	–	–	–	–
Dias et al.	2002	71.283	39.776	–	-0.76	0.12	–

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