UPK 614
0.73
UTI
0.5
CN
1.0
Cdens
0.75
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
6.3 [N/pc2]
- CN 0.5 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 614 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, above 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 age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 231.171 | -53.969 | 1.092 | -1.887 | -4.448 | -6.609 |
| Li et al. | 2025 | 231.204 | -53.967 | 1.098 | -1.85 | -4.488 | â |
| Almeida et al. | 2025 | 231.282 | -53.942 | â | â | â | â |
| Alfonso et al. | 2024 | 231.335 | -53.95 | 1.038 | -1.9 | -4.399 | â |
| Hunt & Reffert | 2024 | 231.148 | -53.979 | 1.085 | -1.869 | -4.462 | -7.497 |
| Cavallo et al. | 2024 | 231.417 | -53.926 | 1.088 | â | â | â |
| Hunt & Reffert | 2023 | 231.148 | -53.979 | 1.085 | -1.869 | -4.462 | -7.497 |
| Almeida et al. | 2023 | 231.291 | -53.933 | â | â | â | â |
| Tarricq et al. | 2022 | 231.341 | -54.036 | 1.101 | -1.899 | -4.44 | â |
| Dias et al. | 2021 | 231.282 | -53.942 | 1.076 | -1.848 | -4.481 | â |
| Cantat-Gaudin et al. | 2020 | 231.204 | -53.967 | 1.098 | -1.85 | -4.488 | â |
| Cantat-Gaudin & Anders | 2020 | 231.211 | -53.966 | 1.084 | -1.851 | -4.477 | â |
| Sim et al. | 2019 | 231.233 | -54.003 | â | -1.84 | -4.48 | 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 | 0.89 | 0.48 | 0.69 | 112 | 0.036 | 113 | 0.6 | â |
| Li et al. | 2025 | 0.89 | 0.47 | â | 79 | 0.155 | â | â | â |
| Almeida et al. | 2025 | 0.92 | 0.70 | â | 147 | â | 107 | â | â |
| Alfonso et al. | 2024 | 0.90 | 0.36 | â | 90 | 0.036 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 113(1) | â | â |
| Cavallo et al. | 2024 | 0.87 | 0.59 | â | 417 | -0.210 | â | â | â |
| Hunt & Reffert | 2023 | 0.89 | 0.39 | 0.69 | 121 | â | â | â | â |
| Almeida et al. | 2023 | 0.89 | 0.49 | â | 297 | -0.011 | 148(1) | 0.60 | â |
| Tarricq et al. | 2022 | 0.87 | â | â | 102 | â | â | â | â |
| Dias et al. | 2021 | 0.92 | 0.70 | â | 147 | 0.036 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.90 | 0.36 | â | 100 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.90 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.89 | â | â | 89 | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.