COIN-Gaia 1
(COIN 1)
0.80
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
13.0 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 1 is a rich, very dense object of very high 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, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a large percentage of members with 2 later reported entries. 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 | 11.82 | 66.747 | 1.552 | -5.04 | -3.146 | -14.34 |
| Li et al. | 2025 | 11.933 | 66.769 | 1.546 | -5.034 | -3.048 | â |
| Almeida et al. | 2025 | 11.999 | 66.782 | â | â | â | â |
| Alfonso et al. | 2024 | 11.803 | 66.687 | 1.51 | -5.006 | -3.114 | â |
| Almeida et al. | 2023 | 11.975 | 66.786 | â | â | â | â |
| He et al. | 2022 | 11.986 | 66.757 | 1.552 | -5.023 | -3.137 | â |
| Dias et al. | 2021 | 11.999 | 66.782 | 1.547 | -5.021 | -3.047 | â |
| Cantat-Gaudin et al. | 2020 | 11.933 | 66.769 | 1.546 | -5.034 | -3.048 | â |
| Cantat-Gaudin & Anders | 2020 | 11.933 | 66.769 | 1.546 | -5.034 | -3.048 | â |
| Monteiro & Dias | 2019 | 11.933 | 66.769 | â | â | â | 2.687 |
| Cantat-Gaudin et al. | 2019 | 11.933 | 66.769 | 1.55 | -5.03 | -3.04 | 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 | 0.64 | 1.5 | â | 224 | 0.035 | 234 | 0.58 | â |
| Li et al. | 2025 | 0.59 | 1.38 | â | 423 | -0.031 | â | â | â |
| Almeida et al. | 2025 | 0.64 | 1.62 | â | 239 | â | 201 | â | â |
| Alfonso et al. | 2024 | 0.66 | 1.13 | â | 224 | 0.035 | â | â | â |
| Almeida et al. | 2023 | 0.63 | 1.67 | â | 198 | 0.004 | 266(1) | 0.58 | â |
| He et al. | 2022 | â | 1.80 | â | 112 | â | â | â | â |
| Tarricq et al. | 2022 | 0.65 | â | â | 200 | â | â | â | â |
| Dias et al. | 2021 | 0.64 | 1.62 | â | 239 | 0.035 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.66 | 1.13 | â | 182 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.63 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 0.67 | 1.29 | â | 543 | 0.036 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 0.64 | 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: good fit. Isochrone match: good fit. Gold sample.