UPK 166
0.85
UTI
0.86
CN
1.0
Cdens
1.0
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
9.7 [N/pc2]
- CN 0.86 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 166 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 339.077 | 46.908 | 1.517 | -0.931 | -3.299 | -11.085 |
| Li et al. | 2025 | 339.203 | 46.927 | 1.508 | -0.907 | -3.229 | â |
| Almeida et al. | 2025 | 339.199 | 46.905 | â | â | â | â |
| Alfonso et al. | 2024 | 339.003 | 46.9 | 1.486 | -0.9 | -3.3 | â |
| Zhang et al. | 2024 | 339.203 | 47.008 | â | â | â | â |
| Hunt & Reffert | 2024 | 339.203 | 47.008 | 1.521 | -0.937 | -3.302 | -10.26 |
| Celli et al. | 2024 | 339.203 | 46.927 | â | â | â | â |
| Cavallo et al. | 2024 | 338.973 | 46.899 | 1.518 | â | â | â |
| Hunt & Reffert | 2023 | 339.203 | 47.008 | 1.521 | -0.937 | -3.302 | -10.26 |
| He et al. | 2022 | 339.075 | 46.965 | 1.5 | -0.908 | -3.279 | â |
| Dias et al. | 2021 | 339.199 | 46.905 | 1.509 | -0.905 | -3.231 | -7.988 |
| Cantat-Gaudin et al. | 2020 | 339.203 | 46.927 | 1.508 | -0.907 | -3.229 | â |
| Cantat-Gaudin & Anders | 2020 | 339.178 | 46.878 | 1.51 | -0.925 | -3.214 | â |
| Sim et al. | 2019 | 339.071 | 46.958 | â | -0.92 | -3.26 | 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 | 0.65 | 0.425 | 0.55 | 32 | -0.001 | 431 | â | â |
| Li et al. | 2025 | 0.67 | 0.41 | â | 34 | 0.142 | â | â | â |
| Almeida et al. | 2025 | 0.62 | 0.44 | â | 45 | â | 431 | â | â |
| Alfonso et al. | 2024 | 0.66 | 0.27 | â | 31 | -0.000 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.063(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 249(1) | â | â |
| Celli et al. | 2024 | â | â | â | 27 | â | 434 | â | â |
| Cavallo et al. | 2024 | 0.69 | 0.62 | â | 10 | -0.060 | â | â | â |
| Hunt & Reffert | 2023 | 0.64 | 0.18 | 0.55 | 16 | â | â | â | â |
| He et al. | 2022 | â | 0.65 | â | 32 | â | â | â | â |
| Dias et al. | 2021 | 0.62 | 0.44 | â | 45 | -0.001 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.66 | 0.27 | â | 27 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.65 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.65 | â | â | 40 | 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.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.