Gulliver 3
0.54
UTI
0.64
CN
0.74
Cdens
0.75
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
78
Core radius and density
1.2 [pc], 3.7 [pc-2]
- CN 0.64 Moderately populated
- Cdens 0.74 Moderately dense
- CC3 0.75 High quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
Gulliver 3 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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 and metallicity parameters (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 122.532 | -37.248 | 0.21 | -2.926 | 4.085 | â |
| Hu & Soubiran | 2025 | 122.525 | -37.255 | â | â | â | â |
| Almeida et al. | 2025 | 122.531 | -37.243 | â | â | â | â |
| Hunt & Reffert | 2024 | 122.533 | -37.248 | 0.209 | -2.922 | 4.083 | â |
| Cavallo et al. | 2024 | 122.525 | -37.255 | 0.209 | â | â | â |
| Hunt & Reffert | 2023 | 122.533 | -37.248 | 0.209 | -2.922 | 4.083 | â |
| Dias et al. | 2021 | 122.531 | -37.243 | 0.174 | -2.939 | 4.112 | â |
| Cantat-Gaudin et al. | 2020 | 122.536 | -37.244 | 0.191 | -2.962 | 4.106 | â |
| Cantat-Gaudin & Anders | 2020 | 122.536 | -37.244 | 0.191 | -2.962 | 4.106 | â |
| Monteiro & Dias | 2019 | 122.536 | -37.244 | â | â | â | 2.94 |
| Cantat-Gaudin et al. | 2018 | 122.536 | -37.244 | 0.191 | -2.962 | 4.106 | 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 | 4.385 | 1.865 | 0.9 | 106 | -0.037 | 434 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.160(5) | â | â | â |
| Almeida et al. | 2025 | 3.64 | 1.99 | â | 81 | â | 326 | â | â |
| Hunt & Reffert | 2024 | 4.34 | 1.85 | 0.90 | 131 | â | 542(1) | â | â |
| Cavallo et al. | 2024 | 3.39 | 1.55 | â | 562 | 0.150 | â | â | â |
| Hunt & Reffert | 2023 | 4.34 | 1.85 | 0.90 | 131 | â | â | â | â |
| Dias et al. | 2021 | 3.64 | 1.99 | â | 81 | -0.100 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.43 | 1.45 | â | 151 | â | â | â | â |
| Kounkel et al. | 2020 | 4.68 | 2.27 | â | 30 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.55 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 9.08 | 1.88 | â | 5 | 0.025 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.55 | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1716, e_all=0.1494.
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg40' along with Gulliver 4.