UPK 168
0.84
UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
12.9 [N/pc2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 168 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 large percentage of members with 2 later reported entries. 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 | 343.75 | 43.321 | 1.665 | -0.528 | -3.997 | -9.911 |
| Li et al. | 2025 | 343.832 | 43.35 | 1.654 | -0.528 | -3.974 | â |
| Almeida et al. | 2025 | 343.756 | 43.409 | â | â | â | â |
| Alfonso et al. | 2024 | -16.57 | 43.404 | 1.644 | -0.568 | -4.031 | â |
| Zhang et al. | 2024 | 344.038 | 43.246 | â | â | â | â |
| Hunt & Reffert | 2024 | 344.038 | 43.246 | 1.67 | -0.575 | -4.056 | -11.446 |
| Cavallo et al. | 2024 | 343.082 | 43.372 | 1.672 | â | â | â |
| Hunt & Reffert | 2023 | 344.038 | 43.246 | 1.67 | -0.575 | -4.056 | -11.446 |
| He et al. | 2022 | 343.854 | 43.293 | 1.657 | -0.527 | -4.017 | â |
| Dias et al. | 2021 | 343.756 | 43.409 | 1.657 | -0.539 | -3.992 | -6.96 |
| Cantat-Gaudin et al. | 2020 | 343.832 | 43.35 | 1.654 | -0.528 | -3.974 | â |
| Cantat-Gaudin & Anders | 2020 | 343.856 | 43.323 | 1.668 | -0.537 | -3.989 | â |
| Sim et al. | 2019 | 343.693 | 43.308 | â | -0.53 | -3.95 | 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 | 0.6 | 0.66 | 0.9 | 36 | 0.090 | 251 | â | â |
| Li et al. | 2025 | 0.64 | 0.53 | â | 30 | 0.249 | â | â | â |
| Almeida et al. | 2025 | 0.59 | 0.72 | â | 63 | â | 238 | â | â |
| Alfonso et al. | 2024 | 0.60 | 0.60 | â | 40 | 0.057 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.091(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 264(1) | â | â |
| Cavallo et al. | 2024 | 0.63 | 0.81 | â | 17 | 0.090 | â | â | â |
| Hunt & Reffert | 2023 | 0.57 | 0.56 | 0.90 | 28 | â | â | â | â |
| He et al. | 2022 | â | 0.80 | â | 35 | â | â | â | â |
| Dias et al. | 2021 | 0.59 | 0.72 | â | 63 | 0.058 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.60 | 0.60 | â | 36 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.59 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.60 | â | â | 45 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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