UPK 119
0.78
UTI
0.61
CN
0.8
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
4.0 [N/pc2]
- CN 0.61 Moderately populated
- Cdens 0.8 Dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 119 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a close distance, near 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 age parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 308.613 | 43.326 | 1.273 | -0.581 | -2.019 | -19.648 |
| Hu & Soubiran | 2025 | 308.588 | 43.336 | â | â | â | â |
| Almeida et al. | 2025 | 308.609 | 43.373 | â | â | â | â |
| Alfonso et al. | 2024 | 308.745 | 43.393 | 1.208 | -0.493 | -1.979 | â |
| Zhang et al. | 2024 | 308.462 | 43.3 | â | â | â | â |
| Hunt & Reffert | 2024 | 308.462 | 43.3 | 1.29 | -0.55 | -2.023 | -22.762 |
| Cavallo et al. | 2024 | 308.588 | 43.336 | 1.28 | â | â | â |
| Hunt & Reffert | 2023 | 308.462 | 43.3 | 1.29 | -0.55 | -2.023 | -22.762 |
| He et al. | 2022 | 308.593 | 43.406 | 1.28 | -0.569 | -2.004 | â |
| Dias et al. | 2021 | 308.609 | 43.373 | 1.281 | -0.621 | -1.99 | â |
| Cantat-Gaudin et al. | 2020 | 308.572 | 43.326 | 1.274 | -0.644 | -1.96 | â |
| Cantat-Gaudin & Anders | 2020 | 308.606 | 43.326 | 1.274 | -0.622 | -1.978 | â |
| Sim et al. | 2019 | 308.56 | 43.377 | â | -0.65 | -2.0 | 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 | 0.77 | 1.31 | 1.69 | 634 | 0.046 | 93 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.110(5) | â | â | â |
| Almeida et al. | 2025 | 0.76 | 1.31 | â | 634 | â | 76 | â | â |
| Alfonso et al. | 2024 | 0.77 | 0.71 | â | 1797 | 0.046 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.023(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 110(1) | â | â |
| Cavallo et al. | 2024 | 0.79 | 1.34 | â | 603 | 0.150 | â | â | â |
| Hunt & Reffert | 2023 | 0.76 | 1.35 | 1.69 | 321 | â | â | â | â |
| He et al. | 2022 | â | 1.45 | â | 891 | â | â | â | â |
| Tarricq et al. | 2022 | 0.75 | â | â | 1622 | â | â | â | â |
| Dias et al. | 2021 | 0.76 | 1.31 | â | 634 | 0.046 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.77 | 0.71 | â | 1549 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.77 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.77 | â | â | 562 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.