HSC 1394

0.16 UTI

0.0

C_N

0.16

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 22

Stellar density (N₅₀/rad) 0.8 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.12 Very low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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HSC 1394 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

⚠️ 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.

Very close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for HSC 1394 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–	70.678	21.927	2.523	8.012	-3.734	8.21
Hu & Soubiran	2025	70.525	21.85	–	–	–	–
Zhang et al.	2024	70.741	21.925	–	–	–	–
Cavallo et al.	2024	70.525	21.85	2.564	–	–	–
Hunt & Reffert	2023	70.741	21.925	2.56	8.1	-3.689	9.989

💡 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–	0.38	1.09	1.23	583	0.011	–	–	–
Hu & Soubiran	2025	–	–	–	–	-0.070⁽⁵⁾	–	–	–
Zhang et al.	2024	–	–	–	–	0.011⁽¹⁾	–	–	–
Cavallo et al.	2024	0.38	1.20	–	589	0.420	–	–	–
Hunt & Reffert	2023	0.38	0.98	1.23	577	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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