COIN-Gaia 25
(COIN 25; FoF 2301)
0.90
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad)
7.1 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
COIN-Gaia 25 is a rich, very dense object of very high 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 age and metallicity parameters (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 | 91.718 | 20.305 | 1.229 | -0.503 | -2.634 | -14.538 |
| Li et al. | 2025 | 91.691 | 20.276 | 1.201 | -0.499 | -2.595 | â |
| Wei et al. | 2025 | 91.673 | 20.237 | 1.223 | -0.518 | -2.673 | â |
| Almeida et al. | 2025 | 91.677 | 20.253 | â | â | â | â |
| Alfonso et al. | 2024 | 91.68 | 20.239 | 1.183 | -0.503 | -2.666 | â |
| Zhang et al. | 2024 | 91.662 | 20.457 | â | â | â | â |
| Hunt & Reffert | 2024 | 91.662 | 20.457 | 1.226 | -0.492 | -2.651 | -13.562 |
| Cavallo et al. | 2024 | 91.66 | 20.272 | 1.228 | â | â | â |
| Hunt & Reffert | 2023 | 91.662 | 20.457 | 1.226 | -0.492 | -2.651 | -13.562 |
| Almeida et al. | 2023 | 91.605 | 20.225 | â | â | â | â |
| He et al. | 2022 | 91.678 | 20.3 | 1.231 | -0.507 | -2.646 | â |
| Tarricq et al. | 2022 | 91.812 | 20.451 | 1.231 | -0.5 | -2.652 | â |
| Dias et al. | 2021 | 91.677 | 20.253 | 1.208 | -0.51 | -2.632 | -14.298 |
| Cantat-Gaudin et al. | 2020 | 91.691 | 20.276 | 1.201 | -0.499 | -2.595 | â |
| Cantat-Gaudin & Anders | 2020 | 91.691 | 20.276 | 1.201 | -0.499 | -2.595 | â |
| Liu & Pang | 2019 | 91.657 | 20.249 | 1.183 | -0.599 | -2.694 | â |
| Monteiro & Dias | 2019 | 91.691 | 20.276 | â | â | â | 2.502 |
| Cantat-Gaudin et al. | 2019 | 91.691 | 20.276 | 1.2 | -0.5 | -2.65 | 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 | 0.81 | 0.61 | 0.71 | 618 | 0.012 | 263 | 0.445 | â |
| Li et al. | 2025 | 0.78 | 0.42 | â | 776 | 0.026 | â | â | â |
| Wei et al. | 2025 | 0.82 | 0.71 | â | 1100 | -0.500 | 416 | 0.44 | â |
| Almeida et al. | 2025 | 0.77 | 0.61 | â | 625 | â | 206 | â | â |
| Alfonso et al. | 2024 | 0.82 | 0.38 | â | 781 | 0.012 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.100(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 215(1) | â | â |
| Cavallo et al. | 2024 | 0.82 | 0.65 | â | 490 | 0.310 | â | â | â |
| Hunt & Reffert | 2023 | 0.77 | 0.36 | 0.71 | 574 | â | â | â | â |
| Almeida et al. | 2023 | 0.79 | 0.66 | â | 618 | -0.046 | 311(1) | 0.45 | â |
| He et al. | 2022 | â | 0.85 | â | 316 | â | â | â | â |
| Tarricq et al. | 2022 | 0.81 | â | â | 603 | â | â | â | â |
| Dias et al. | 2021 | 0.77 | 0.61 | â | 625 | 0.012 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.82 | 0.38 | â | 562 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.81 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1180 | -0.500 | â | â | â |
| Monteiro & Dias | 2019 | 0.86 | 0.62 | â | 557 | 0.022 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 0.81 | 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.
Cavallo et al. (2024)
Gold sample.