UPK 535
(OCSN 312)
0.85
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
6.0 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 535 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (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 | 126.935 | -50.797 | 3.113 | -12.906 | 3.281 | 10.7 |
| Li et al. | 2025 | 127.025 | -50.899 | 3.086 | -12.913 | 3.217 | â |
| Wei et al. | 2025 | 127.503 | -50.597 | 3.06 | -12.75 | 3.166 | â |
| Almeida et al. | 2025 | 127.112 | -50.941 | â | â | â | â |
| Alfonso et al. | 2024 | 126.874 | -50.76 | 3.081 | -12.916 | 3.318 | â |
| Cavallo et al. | 2024 | 126.734 | -50.645 | 3.148 | â | â | â |
| Hunt & Reffert | 2023 | 126.568 | -50.083 | 3.15 | -13.025 | 3.345 | 3.91 |
| Almeida et al. | 2023 | 127.427 | -50.858 | â | â | â | â |
| Qin et al. | 2023 | 126.88 | -50.66 | 3.12 | -12.72 | 3.34 | 10.06 |
| He et al. | 2022 | 127.025 | -50.782 | 3.147 | -12.986 | 3.317 | â |
| Dias et al. | 2021 | 127.112 | -50.941 | 3.084 | -12.932 | 3.176 | 11.303 |
| Cantat-Gaudin et al. | 2020 | 127.025 | -50.899 | 3.086 | -12.913 | 3.217 | â |
| Cantat-Gaudin & Anders | 2020 | 127.042 | -50.896 | 3.095 | -12.955 | 3.173 | â |
| Sim et al. | 2019 | 127.06 | -51.092 | â | -13.08 | 3.25 | 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 | 0.32 | 0.28 | 0.47 | 32 | -0.029 | 124 | 0.57 | â |
| Li et al. | 2025 | 0.38 | 0.23 | â | 38 | 0.050 | â | â | â |
| Wei et al. | 2025 | 0.32 | 0.61 | â | 6 | -0.250 | 124 | 0.66 | â |
| Almeida et al. | 2025 | 0.32 | 0.33 | â | 43 | â | 120 | â | â |
| Alfonso et al. | 2024 | 0.32 | 0.07 | â | 26 | -0.029 | â | â | â |
| Cavallo et al. | 2024 | 0.32 | 0.58 | â | 17 | -0.090 | â | â | â |
| Hunt & Reffert | 2023 | 0.31 | 0.14 | 0.47 | 22 | â | â | â | â |
| Almeida et al. | 2023 | 0.32 | 0.25 | â | 53 | 0.056 | 209(1) | 0.48 | â |
| Qin et al. | 2023 | 0.35 | 0.28 | â | 25 | â | â | â | â |
| He et al. | 2022 | â | 0.40 | â | 32 | â | â | â | â |
| Dias et al. | 2021 | 0.32 | 0.33 | â | 43 | -0.029 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.32 | 0.07 | â | 33 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.32 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.32 | 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.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.