UBC 1443
0.49
UTI
0.46
CN
0.62
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad)
3.1 [N/pc2]
- CN 0.46 Poorly populated
- Cdens 0.62 Moderately dense
- CC3 0.75 High quality
- Clit 0.3 Poorly studied
- Cdup 1.0 Unique
Overview
UBC 1443 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant 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 | 136.729 | -40.867 | 0.272 | -5.684 | 4.065 | 36.787 |
| Hu & Soubiran | 2025 | 136.751 | -40.873 | â | â | â | â |
| Hunt & Reffert | 2024 | 136.713 | -40.862 | 0.276 | -5.671 | 4.066 | 36.148 |
| Cavallo et al. | 2024 | 136.751 | -40.873 | 0.28 | â | â | â |
| Hunt & Reffert | 2023 | 136.713 | -40.862 | 0.276 | -5.671 | 4.066 | 36.148 |
| Castro-Ginard et al. | 2022 | 136.75 | -40.88 | 0.27 | -5.68 | 4.07 | 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 | 3.26 | 1.21 | 1.62 | 681 | 0.015 | 341 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.160(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 341(1) | â | â |
| Cavallo et al. | 2024 | 2.82 | 1.21 | â | 1148 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 3.26 | 1.51 | 1.62 | 681 | â | â | â | â |
| Castro-Ginard et al. | 2022 | 3.61 | 1.17 | â | 640 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.