UPK 418
0.26
UTI
0.0
CN
0.13
Cdens
0.25
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
0.7 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.13 Very loose
- CC3 0.25 Low quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
UPK 418 is a sparse, very loose object of low 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, young cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 112.565 | 5.58 | 1.017 | -2.629 | -1.112 | 36.308 |
| Almeida et al. | 2025 | 112.5 | 5.576 | â | â | â | â |
| Alfonso et al. | 2024 | 112.615 | 5.705 | 1.14 | -2.666 | -1.555 | â |
| Almeida et al. | 2023 | 112.476 | 5.579 | â | â | â | â |
| Dias et al. | 2021 | 112.5 | 5.576 | 1.116 | -2.643 | -1.146 | â |
| Cantat-Gaudin et al. | 2020 | 112.48 | 5.605 | 1.111 | -2.646 | -0.983 | â |
| Cantat-Gaudin & Anders | 2020 | 112.39 | 5.557 | 1.12 | -2.651 | -1.17 | â |
| Sim et al. | 2019 | 112.561 | 5.618 | â | -2.68 | -1.6 | 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 | 0.87 | 0.06 | â | 89 | -0.220 | 104 | 0.49 | â |
| Almeida et al. | 2025 | 0.87 | 0.20 | â | 197 | â | 76 | â | â |
| Alfonso et al. | 2024 | 0.92 | 0.01 | â | 17 | -0.220 | â | â | â |
| Almeida et al. | 2023 | 0.82 | 0.06 | â | 100 | -0.068 | 131(1) | 0.49 | â |
| Tarricq et al. | 2022 | 0.90 | â | â | 63 | â | â | â | â |
| Dias et al. | 2021 | 0.87 | 0.20 | â | 197 | -0.220 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.92 | 0.01 | â | 63 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.87 | â | â | â | â | â | â | â |
| Sim et al. | 2019 | 0.83 | 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.