HSC 1480
0.22
UTI
0.27
CN
0.06
Cdens
0.62
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
27
Core radius and density
2.1 [pc], 0.3 [pc-2]
- CN 0.27 Poorly populated
- Cdens 0.06 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
HSC 1480 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age 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 | 91.414 | 23.516 | 0.171 | 0.266 | -0.416 | â |
| Zhang et al. | 2024 | 91.429 | 23.511 | â | â | â | â |
| Hunt & Reffert | 2024 | 91.429 | 23.511 | 0.185 | 0.274 | -0.429 | â |
| Cavallo et al. | 2024 | 91.411 | 23.506 | 0.185 | â | â | â |
| Hunt & Reffert | 2023 | 91.429 | 23.511 | 0.185 | 0.274 | -0.429 | 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 | 4.68 | 2.08 | 2.505 | 44 | 0.300 | 688 | â | â |
| Hunt & Reffert | 2024 | 4.68 | 2.08 | 2.51 | 44 | â | 688(1) | â | â |
| Cavallo et al. | 2024 | 4.13 | 1.37 | â | 263 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 4.68 | 2.08 | 2.50 | 44 | 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 classes: 0.66 (50th percentile), true positive (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.66 (50th percentile), true positive (human-assigned).