NGC 3590

(FoF 237)

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.78 1.0 1.0 1.0 1.0 NGC 3590 is a rich, very dense object of very high C3 quality. It is very well-studied in the literature. This object shares a large percentage of members with a later reported entry.
C3	N_50	r_50
AA	173	1.6

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Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dambis (1999)	168.246	-60.788	–	–	–	–
Dias et al. (2002)	168.246	-60.788	–	-3.3	-1.28	-7.33
Kharchenko et al. (2012)	168.258	-60.775	–	-6.61	1.55	–
Loktin & Popova (2017)	168.24	-60.788	–	-3.3	-1.28	-7.3
Liu & Pang (2019)	168.249	-60.777	0.355	-6.108	1.224	–
Cantat-Gaudin et al. (2020)	168.262	-60.79	0.361	-6.1	1.013	–
Dias et al. (2021)	168.262	-60.788	0.362	-6.116	1.023	–
Jaehnig et al. (2021)	168.244	-60.789	0.397	-6.082	1.052	–
Hunt & Reffert (2023)	168.258	-60.79	0.384	-6.121	1.038	–
Cavallo et al. (2024)	168.263	-60.784	0.384	–	–	–
Hunt & Reffert (2024)	168.258	-60.79	0.384	-6.121	1.038	–
UCC	168.263	-60.79	0.377	-6.106	1.038	–

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Estimated members

1 2 3

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Fundamental parameters

Reference	Values
Dambis (1999)	E_B-V_=0.535, DM0=11.7, log_age_=7.2
Dias et al. (2002)	E(B-V)=0.449, Dist=1651.0, Age=7.231
Kharchenko et al. (2012)	e_bv=0.416, distance=1660, log_age=7.4
Loktin & Popova (2017)	E(B-V)=0.449, Dmod=11.089, logt=7.231
Liu & Pang (2019)	Age=0.007, Z=0.5
Cantat-Gaudin et al. (2020)	AVNN=1.3, DMNN=12.11, AgeNN=7.42
Dias et al. (2021)	Av=1.662, Dist=2420, logage=7.147, [Fe/H]=0.058
Hunt & Reffert (2023)	AV50=1.424, diffAV50=2.013, MOD50=11.906, logAge50=7.338
Cavallo et al. (2024)	AV50=1.55, dMod50=11.82, logAge50=7.24, [Fe/H]50=0.01
Hunt & Reffert (2024)	MassJ=956.648

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Cluster region

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
DBSB 61	100.0	168.26	-60.79	0.38	-6.11	1.05	–	0.1