NGC 2467

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.0 0.05 0.5 0.8 1.0 NGC 2467 is a sparse, very loose object of intermediate C3 quality. It is well-studied in the literature. This object shares a large percentage of members with a later reported entry. Warning: contains less than 25 stars with P>0.5 estimated.
C3	N_50	r_50
BB	19	6.7

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Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dambis (1999)	118.08	-26.442	–	–	–	–
Dias et al. (2002)	118.108	-26.437	–	-3.65	2.68	58.24
Chen et al. (2003)	118.088	-26.363	–	-5.82	1.63	66.0
Loktin & Popova (2017)	118.11	-26.436	–	–	–	55.8
Jaehnig et al. (2021)	118.18	-26.374	0.191	-2.554	2.578	–
Hunt & Reffert (2023)	117.997	-26.411	0.216	-1.49	2.453	77.739
Cavallo et al. (2024)	117.925	-26.383	0.216	–	–	–
Hunt & Reffert (2024)	117.997	-26.411	0.216	-1.49	2.453	77.739
UCC	117.969	-26.408	0.214	-1.486	2.45	77.88

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Estimated members

1 2

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Fundamental parameters

Reference	Values
Dambis (1999)	E_B-V_=0.298, DM0=10.5, log_age_=7.7
Dias et al. (2002)	E(B-V)=0.338, Dist=1355.0, Age=7.103
Chen et al. (2003)	HDis=1355, Age=0.01
Loktin & Popova (2017)	E(B-V)=0.338, Dmod=10.66, logt=7.103
Hunt & Reffert (2023)	AV50=0.734, diffAV50=1.192, MOD50=13.295, logAge50=8.394
Cavallo et al. (2024)	AV50=0.47, dMod50=12.9, logAge50=8.46, [Fe/H]50=0.43
Hunt & Reffert (2024)	MassJ=101.727

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Cluster region

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1615	76.0	117.95	-26.34	0.22	-1.48	2.44	77.88	0.03