COIN-Gaia 9
(COIN 9)
0.79
UTI
0.6
CN
1.0
Cdens
0.75
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
7.2 [N/pc2]
- CN 0.6 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 9 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-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 | 47.716 | 48.025 | 1.15 | -2.026 | -2.866 | -14.148 |
| Li et al. | 2025 | 47.748 | 48.023 | 1.119 | -1.934 | -2.81 | â |
| Almeida et al. | 2025 | 47.812 | 48.022 | â | â | â | â |
| Alfonso et al. | 2024 | 48.196 | 47.805 | 1.094 | -2.075 | -3.047 | â |
| Zhang et al. | 2024 | 47.714 | 48.03 | â | â | â | â |
| Hunt & Reffert | 2024 | 47.714 | 48.03 | 1.113 | -2.035 | -3.073 | -14.035 |
| Cavallo et al. | 2024 | 49.166 | 47.486 | 1.113 | â | â | â |
| Hunt & Reffert | 2023 | 47.714 | 48.03 | 1.113 | -2.035 | -3.073 | -14.035 |
| Almeida et al. | 2023 | 47.738 | 47.971 | â | â | â | â |
| He et al. | 2022 | 47.734 | 48.038 | 1.159 | -2.066 | -2.907 | â |
| Dias et al. | 2021 | 47.812 | 48.022 | 1.138 | -1.932 | -2.792 | -3.054 |
| Cantat-Gaudin et al. | 2020 | 47.748 | 48.023 | 1.119 | -1.934 | -2.81 | â |
| Cantat-Gaudin & Anders | 2020 | 47.748 | 48.023 | 1.119 | -1.934 | -2.81 | â |
| Monteiro & Dias | 2019 | 47.748 | 48.023 | â | â | â | 2.716 |
| Cantat-Gaudin et al. | 2019 | 47.748 | 48.023 | 1.12 | -1.93 | -2.79 | 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 | 0.855 | 1.19 | 1.33 | 118 | 0.000 | 162 | 0.48 | â |
| Li et al. | 2025 | 0.81 | 1.16 | â | 85 | -0.031 | â | â | â |
| Almeida et al. | 2025 | 0.83 | 1.22 | â | 118 | â | 120 | â | â |
| Alfonso et al. | 2024 | 0.86 | 0.57 | â | 217 | 0.054 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.092(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 227(1) | â | â |
| Cavallo et al. | 2024 | 0.94 | 1.29 | â | 78 | -0.010 | â | â | â |
| Hunt & Reffert | 2023 | 0.85 | 0.93 | 1.33 | 150 | â | â | â | â |
| Almeida et al. | 2023 | 0.85 | 1.22 | â | 188 | 0.000 | 162(1) | 0.48 | â |
| He et al. | 2022 | â | 1.30 | â | 63 | â | â | â | â |
| Tarricq et al. | 2022 | 0.84 | â | â | 166 | â | â | â | â |
| Dias et al. | 2021 | 0.83 | 1.22 | â | 118 | 0.053 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.86 | 0.57 | â | 158 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.87 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 0.98 | 1.11 | â | 70 | 0.022 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 0.87 | â | â | â | 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.