HSC 1548
0.14
UTI
0.0
CN
0.17
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
23
Core radius and density
1.8 [pc], 0.9 [pc-2]
- CN 0.0 Sparse
- Cdens 0.17 Very loose
- CC3 0.38 Low quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1548 is a sparse, very loose 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.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 92.214 | 13.899 | 0.174 | 0.278 | -0.511 | â |
| Hu & Soubiran | 2025 | 92.197 | 13.938 | â | â | â | â |
| Hunt & Reffert | 2024 | 92.21 | 13.897 | 0.176 | 0.212 | -0.422 | â |
| Cavallo et al. | 2024 | 92.197 | 13.938 | 0.175 | â | â | â |
| Hunt & Reffert | 2023 | 92.21 | 13.897 | 0.176 | 0.212 | -0.422 | â |
đĄ 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 | 99999â | 4.62 | 2.8 | 2.37 | 242 | 0.045 | 759 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.400(5) | â | â | â |
| Hunt & Reffert | 2024 | 4.62 | 2.80 | 2.37 | 241 | â | 759(1) | â | â |
| Cavallo et al. | 2024 | 4.53 | 2.38 | â | 603 | 0.490 | â | â | â |
| Hunt & Reffert | 2023 | 4.62 | 2.80 | 2.37 | 242 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.07 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.07 (50th percentile).