UPK 167
0.66
UTI
0.58
CN
0.65
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
28.6 [arcmin]
- CN 0.58 Moderately populated
- Cdens 0.65 Moderately dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 167 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low 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 is moderately studied in the literature.
Close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 336.904 | 49.792 | 1.842 | 1.582 | -0.126 | -11.345 |
| Li et al. | 2025 | 337.143 | 49.814 | 1.82 | 1.549 | -0.029 | â |
| Almeida et al. | 2025 | 337.324 | 49.895 | â | â | â | â |
| Alfonso et al. | 2024 | 336.948 | 49.92 | 1.777 | 1.56 | -0.143 | â |
| Hunt & Reffert | 2024 | 336.662 | 49.516 | 1.796 | 1.54 | -0.138 | -12.724 |
| Cavallo et al. | 2024 | 337.145 | 49.933 | 1.802 | â | â | â |
| Hunt & Reffert | 2023 | 336.662 | 49.516 | 1.796 | 1.54 | -0.138 | -12.724 |
| Tarricq et al. | 2022 | 336.479 | 49.774 | 1.858 | 1.585 | -0.157 | â |
| Dias et al. | 2021 | 337.324 | 49.895 | 1.803 | 1.584 | -0.003 | -15.903 |
| Cantat-Gaudin et al. | 2020 | 337.143 | 49.814 | 1.82 | 1.549 | -0.029 | â |
| Cantat-Gaudin & Anders | 2020 | 337.163 | 49.811 | 1.801 | 1.556 | -0.013 | â |
| Sim et al. | 2019 | 336.909 | 49.758 | â | 1.56 | -0.09 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.63 | 0.49 | â | 103 | 0.159 | â | â | â |
| Almeida et al. | 2025 | 0.54 | 0.46 | â | 282 | â | 328 | â | â |
| Alfonso et al. | 2024 | 0.56 | 0.40 | â | 191 | -0.065 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 105* | â | â |
| Cavallo et al. | 2024 | 0.55 | 0.57 | â | 141 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 0.52 | 0.23 | 0.76 | 124 | â | â | â | â |
| Tarricq et al. | 2022 | 0.55 | â | â | 129 | â | â | â | â |
| Dias et al. | 2021 | 0.54 | 0.46 | â | 282 | -0.065 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.56 | 0.40 | â | 123 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.55 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.55 | â | â | 100 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.