UPK 537
0.37
UTI
0.0
CN
0.18
Cdens
0.38
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
29.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.18 Very loose
- CC3 0.38 Low quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
UPK 537 is a sparse, very loose object of low 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, 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.
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 | 126.846 | -52.065 | 1.656 | -6.659 | 7.74 | 16.587 |
| Li et al. | 2025 | 126.57 | -52.113 | 1.652 | -6.638 | 7.765 | â |
| Almeida et al. | 2025 | 126.645 | -52.013 | â | â | â | â |
| Alfonso et al. | 2024 | 126.646 | -51.705 | 1.619 | -6.566 | 7.723 | â |
| Cavallo et al. | 2024 | 126.376 | -51.726 | 1.64 | â | â | â |
| Hunt & Reffert | 2023 | 125.646 | -51.569 | 1.637 | -6.492 | 7.716 | 18.409 |
| Almeida et al. | 2023 | 126.879 | -52.022 | â | â | â | â |
| Tarricq et al. | 2022 | 127.129 | -52.308 | 1.659 | -6.669 | 7.714 | â |
| Dias et al. | 2021 | 126.645 | -52.013 | 1.655 | -6.522 | 7.803 | -3.864 |
| Cantat-Gaudin et al. | 2020 | 126.57 | -52.113 | 1.652 | -6.638 | 7.765 | â |
| Cantat-Gaudin & Anders | 2020 | 126.669 | -52.05 | 1.649 | -6.576 | 7.757 | â |
| Sim et al. | 2019 | 126.792 | -51.97 | â | -6.69 | 7.58 | 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 | 0.52 | 0.33 | â | 284 | -0.058 | â | â | â |
| Almeida et al. | 2025 | 0.59 | 0.71 | â | 105 | â | 108 | â | â |
| Alfonso et al. | 2024 | 0.63 | 0.54 | â | 224 | 0.082 | â | â | â |
| Cavallo et al. | 2024 | 0.63 | 0.89 | â | 41 | 0.390 | â | â | â |
| Hunt & Reffert | 2023 | 0.58 | 0.70 | 1.61 | 62 | â | â | â | â |
| Almeida et al. | 2023 | 0.59 | 0.70 | â | 222 | 0.053 | 243* | 0.78 | â |
| Tarricq et al. | 2022 | 0.62 | â | â | 234 | â | â | â | â |
| Dias et al. | 2021 | 0.59 | 0.71 | â | 105 | 0.082 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.63 | 0.54 | â | 234 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.60 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.60 | â | â | 40 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.