HSC 1548

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0.29 UTI
0.0
CN
0.57
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.8 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.57 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1548 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a large 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.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 92.214 13.899 0.174 0.278 -0.511 –
Hu & Soubiran 2025 92.197 13.938 – – – –
Hunt & Reffert 2024 92.21 13.897 0.176 0.212 -0.422 –
Cavallo et al. 2024 92.197 13.938 0.175 – – –
Hunt & Reffert 2023 92.21 13.897 0.176 0.212 -0.422 –

💡 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] Bfrac BSS
UCC 99999– 4.575 2.59 2.37 422 0.045 759 – –
Hu & Soubiran 2025 – – – – -0.400(5) – – –
Hunt & Reffert 2024 – – – – – 759(1) – –
Cavallo et al. 2024 4.53 2.38 – 603 0.490 – – –
Hunt & Reffert 2023 4.62 2.80 2.37 242 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3891 80.0 92.21 13.9 0.18 0.31 -0.53 – 0.04

💡 Note: The % column shows the percentage of members that HSC 1548 shares with each listed object.

Visualization

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