NGC 3572

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.76 1.0 1.0 1.0 1.0 NGC 3572 is a rich, very dense object of very high C3 quality. It is very well-studied in the literature. This object shares a small percentage of members with at least one entry reported in the same catalogue.
C3	N_50	r_50
AA	122	3.7

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Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dambis (1999)	167.596	-60.248	–	–	–	–
Dias et al. (2002)	167.596	-60.248	–	-4.37	-0.96	-4.0
Kharchenko et al. (2012)	167.602	-60.25	–	-9.19	2.31	–
Loktin & Popova (2017)	167.595	-60.248	–	-4.37	-0.96	-8.0
Cantat-Gaudin et al. (2020)	167.64	-60.294	0.376	-6.261	1.893	–
Dias et al. (2021)	167.633	-60.302	0.383	-6.266	1.904	–
Jaehnig et al. (2021)	167.646	-60.293	0.409	-6.204	1.921	–
Hunt & Reffert (2023)	167.625	-60.28	0.373	-6.253	1.949	-4.931
Cavallo et al. (2024)	167.639	-60.302	0.371	–	–	–
Hunt & Reffert (2024)	167.625	-60.28	0.373	-6.253	1.949	-4.931
UCC	167.655	-60.311	0.381	-6.245	1.904	-4.918

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Estimated members

1 2 3

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Fundamental parameters

Reference	Values
Dambis (1999)	E_B-V_=0.44, DM0=11.9, log_age_=6.5
Dias et al. (2002)	E(B-V)=0.389, Dist=1995.0, Age=6.891
Kharchenko et al. (2012)	e_bv=0.364, distance=1997, log_age=6.925
Loktin & Popova (2017)	E(B-V)=0.387, Dmod=11.51, logt=6.896
Cantat-Gaudin et al. (2020)	AVNN=1.53, DMNN=11.95, AgeNN=6.68
Dias et al. (2021)	Av=1.435, Dist=2276, logage=6.811, [Fe/H]=0.071
Hunt & Reffert (2023)	AV50=1.292, diffAV50=1.501, MOD50=11.921, logAge50=6.687
Cavallo et al. (2024)	AV50=1.42, dMod50=11.75, logAge50=6.58, [Fe/H]50=-0.18
Hunt & Reffert (2024)	MassJ=502.358

Search coordinates in Bayestar19

Cluster region

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 227	16.4	167.49	-60.31	0.37	-6.22	1.85	-28.47	0.15
Hogg 10	14.8	167.68	-60.41	0.39	-6.2	1.79	-10.87	0.77