UPK 265
0.45
UTI
0.0
CN
0.38
Cdens
0.38
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
1.9 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.38 Loose
- CC3 0.38 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
UPK 265 is a sparse, loose object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. 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 | 31.922 | 65.448 | 1.16 | -0.533 | -0.437 | -4.616 |
| Li et al. | 2025 | 31.915 | 65.449 | 1.131 | -0.518 | -0.412 | â |
| Almeida et al. | 2025 | 32.029 | 65.43 | â | â | â | â |
| Alfonso et al. | 2024 | 32.605 | 65.295 | 1.142 | -0.598 | -0.545 | â |
| Hunt & Reffert | 2024 | 31.506 | 65.459 | 1.156 | -0.518 | -0.468 | -8.691 |
| Cavallo et al. | 2024 | 32.179 | 65.425 | 1.154 | â | â | â |
| Hunt & Reffert | 2023 | 31.506 | 65.459 | 1.156 | -0.518 | -0.468 | -8.691 |
| Almeida et al. | 2023 | 31.997 | 65.343 | â | â | â | â |
| He et al. | 2022 | 31.642 | 65.476 | 1.16 | -0.542 | -0.424 | â |
| Tarricq et al. | 2022 | 31.923 | 65.464 | 1.156 | -0.581 | -0.432 | â |
| Dias et al. | 2021 | 32.029 | 65.43 | 1.135 | -0.52 | -0.39 | â |
| Cantat-Gaudin et al. | 2020 | 31.915 | 65.449 | 1.131 | -0.518 | -0.412 | â |
| Cantat-Gaudin & Anders | 2020 | 31.907 | 65.449 | 1.136 | -0.508 | -0.378 | â |
| Sim et al. | 2019 | 31.735 | 65.461 | â | -0.51 | -0.37 | 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 | 0.86 | 1.95 | 2.0 | 87 | -0.116 | 195 | 0.75 | â |
| Li et al. | 2025 | 0.78 | 1.77 | â | 439 | -0.235 | â | â | â |
| Almeida et al. | 2025 | 0.85 | 1.95 | â | 26 | â | 195 | â | â |
| Alfonso et al. | 2024 | 0.89 | 1.36 | â | 117 | -0.116 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 159(1) | â | â |
| Cavallo et al. | 2024 | 0.98 | 2.07 | â | 68 | 0.370 | â | â | â |
| Hunt & Reffert | 2023 | 0.81 | 1.90 | 2.00 | 50 | â | â | â | â |
| Almeida et al. | 2023 | 0.83 | 2.10 | â | 210 | -0.176 | 235(1) | 0.75 | â |
| He et al. | 2022 | â | 2.35 | â | 25 | â | â | â | â |
| Tarricq et al. | 2022 | 0.87 | â | â | 93 | â | â | â | â |
| Dias et al. | 2021 | 0.85 | 1.95 | â | 26 | -0.116 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.89 | 1.36 | â | 87 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.86 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.86 | â | â | 398 | 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.