Pickard 160

0.07 UTI

0.26

C_N

0.45

C_dens

0.75

C_C3

0.0

C_lit

0.23

C_dup

N₅₀ (P>50% members) 26

Stellar density (N₅₀/rad) 2.2 [N/pc²]

C3 classification AB

C_N 0.26 Poorly populated
C_dens 0.45 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.23 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Pickard 160 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~6.89 kpc) differs significantly from the median photometric distance (~4.55 kpc).

Distant Moderate extinction Near-solar metallicity Very young

Data

🔍 Search references for Pickard 160 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	115.009	-23.521	0.145	-1.518	2.364	59.583
Dias et al.	2026	115.003	-23.539	0.159	-1.444	2.313	–

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

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	4.55	1.44	–	19	-0.330	–	–	–
Dias et al.	2026	4.55	1.44	–	19	-0.330	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3677	76.9	115.01	-23.51	0.16	-1.54	2.39	81.78	0.37

💡 Note: The % column shows the percentage of members that Pickard 160 shares with each listed object.

Visualization

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