HSC 1496

0.29 UTI

0.0

C_N

0.1

C_dens

0.75

C_C3

0.31

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 21

Radius (P>50% members) 3.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.75 High 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 1496 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large^* distance, well 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.

(*): The parallax distance estimate (~7.52 kpc) differs significantly from the median photometric distance (~5.70 kpc).

Very distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HSC 1496 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	–	86.428	19.063	0.133	0.749	-0.398	21.837
Hu & Soubiran	2025	86.424	19.065	–	–	–	–
Zhang et al.	2024	86.436	19.043	–	–	–	–
Hunt & Reffert	2024	86.436	19.043	0.133	0.757	-0.385	-0.906
Cavallo et al.	2024	86.424	19.065	0.132	–	–	–
Hunt & Reffert	2023	86.436	19.043	0.133	0.757	-0.385	-0.906

💡 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	–	–	–	–	-0.320*	–	–	–
Zhang et al.	2024	–	–	–	–	-0.321*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	338*	–	–
Cavallo et al.	2024	3.78	0.57	–	1660	0.120	–	–	–
Hunt & Reffert	2023	7.61	1.71	0.78	318	–	–	–	–

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

Visualization

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