HSC 1487

0.28 UTI

0.26

C_N

0.4

C_dens

0.12

C_C3

0.31

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 26

Radius (P>50% members) 2.8 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.4 Loose
C_C3 0.12 Very low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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HSC 1487 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate distance, above 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.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1487 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	–	92.838	23.647	0.227	0.895	-0.264	31.975
Hu & Soubiran	2025	92.847	23.664	–	–	–	–
Zhang et al.	2024	92.846	23.649	–	–	–	–
Hunt & Reffert	2024	92.846	23.649	0.225	0.925	-0.3	40.441
Cavallo et al.	2024	92.847	23.664	0.218	–	–	–
Hunt & Reffert	2023	92.846	23.649	0.225	0.925	-0.3	40.441

💡 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]	Bfr	BSS
Hu & Soubiran	2025	–	–	–	–	-0.250*	–	–	–
Zhang et al.	2024	–	–	–	–	-0.229*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	195*	–	–
Cavallo et al.	2024	3.65	1.78	–	631	0.140	–	–	–
Hunt & Reffert	2023	3.99	1.59	1.44	875	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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