COIN-Gaia 5
(COIN 5)
0.63
UTI
0.32
CN
0.94
Cdens
0.38
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
9.8 [arcmin]
- CN 0.32 Poorly populated
- Cdens 0.94 Very dense
- CC3 0.38 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 5 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a close distance, near 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 metallicity parameter (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 | 27.408 | 58.079 | 1.093 | -2.809 | -0.558 | -29.97 |
| Li et al. | 2025 | 27.408 | 58.078 | 1.063 | -2.774 | -0.511 | â |
| Almeida et al. | 2025 | 27.349 | 58.072 | â | â | â | â |
| Alfonso et al. | 2024 | 27.408 | 58.063 | 1.062 | -2.81 | -0.572 | â |
| Hunt & Reffert | 2024 | 27.463 | 58.05 | 1.09 | -2.857 | -0.6 | -47.582 |
| Cavallo et al. | 2024 | 27.231 | 58.031 | 1.092 | â | â | â |
| Hunt & Reffert | 2023 | 27.463 | 58.05 | 1.09 | -2.857 | -0.6 | -47.582 |
| He et al. | 2022 | 27.406 | 58.044 | 1.107 | -2.821 | -0.611 | â |
| Tarricq et al. | 2022 | 27.408 | 58.001 | 1.099 | -2.847 | -0.57 | â |
| Dias et al. | 2021 | 27.349 | 58.072 | 1.09 | -2.8 | -0.503 | -23.966 |
| Cantat-Gaudin et al. | 2020 | 27.408 | 58.078 | 1.063 | -2.774 | -0.511 | â |
| Cantat-Gaudin & Anders | 2020 | 27.408 | 58.078 | 1.063 | -2.774 | -0.511 | â |
| Monteiro & Dias | 2019 | 27.408 | 58.078 | â | â | â | 2.77 |
| Cantat-Gaudin et al. | 2019 | 27.408 | 58.078 | 1.06 | -2.77 | -0.53 | 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 | 0.91 | 0.69 | 0.61 | 151 | 0.019 | 105 | â | â |
| Li et al. | 2025 | 1.09 | 0.69 | â | 52 | 0.019 | â | â | â |
| Almeida et al. | 2025 | 0.85 | 0.85 | â | 201 | â | 110 | â | â |
| Alfonso et al. | 2024 | 0.91 | 0.45 | â | 115 | -0.167 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 100(1) | â | â |
| Cavallo et al. | 2024 | 0.92 | 0.80 | â | 219 | 0.360 | â | â | â |
| Hunt & Reffert | 2023 | 0.87 | 0.62 | 0.61 | 225 | â | â | â | â |
| He et al. | 2022 | â | 1.05 | â | 71 | â | â | â | â |
| Tarricq et al. | 2022 | 0.89 | â | â | 115 | â | â | â | â |
| Dias et al. | 2021 | 0.85 | 0.85 | â | 201 | -0.167 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.91 | 0.45 | â | 110 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.92 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 0.92 | 0.51 | â | 187 | 0.028 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 0.92 | â | â | â | â | â | â | â |
(N): Indicates that are N extra values assigned to this parameter in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.