Gulliver 4
(FoF 100)
0.67
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.42
Clit
1.0
Cdup
Stellar density (N50/rad)
8.5 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.42 Poorly studied
- Cdup 1.0 Unique
Overview
Gulliver 4 is a rich, very 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, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 122.149 | -37.501 | 0.322 | -2.893 | 3.065 | 53.21 |
| Hu & Soubiran | 2025 | 122.151 | -37.492 | â | â | â | â |
| Almeida et al. | 2025 | 122.167 | -37.484 | â | â | â | â |
| Hunt & Reffert | 2024 | 122.171 | -37.505 | 0.326 | -2.889 | 3.055 | 51.653 |
| Cavallo et al. | 2024 | 122.151 | -37.492 | 0.327 | â | â | â |
| Hunt & Reffert | 2023 | 122.171 | -37.505 | 0.326 | -2.889 | 3.055 | 51.653 |
| Jadhav & Subramaniam | 2021 | 122.164 | -37.5 | â | â | â | â |
| Rain et al. | 2021 | 122.164 | -37.5 | 0.3 | -2.912 | 3.033 | â |
| Dias et al. | 2021 | 122.167 | -37.484 | 0.299 | -2.921 | 3.034 | 52.425 |
| Cantat-Gaudin et al. | 2020 | 122.164 | -37.5 | 0.3 | -2.912 | 3.033 | â |
| Cantat-Gaudin & Anders | 2020 | 122.164 | -37.5 | 0.3 | -2.912 | 3.033 | â |
| Liu & Pang | 2019 | 122.177 | -37.513 | 0.289 | -2.829 | 3.038 | â |
| Monteiro & Dias | 2019 | 122.164 | -37.5 | â | â | â | 2.532 |
| Soubiran et al. | 2018 | 122.164 | -37.5 | â | â | â | 51.98 |
| Cantat-Gaudin et al. | 2018 | 122.164 | -37.5 | 0.3 | -2.912 | 3.033 | 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 | 2.75 | 1.62 | 2.32 | 1164 | -0.130 | 496 | â | 2 |
| Hu & Soubiran | 2025 | â | â | â | â | -0.130(5) | â | â | â |
| Almeida et al. | 2025 | 2.67 | 1.92 | â | 1208 | â | 320 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 830(1) | â | â |
| Cavallo et al. | 2024 | 2.59 | 1.62 | â | 891 | 0.310 | â | â | â |
| Hunt & Reffert | 2023 | 2.76 | 1.85 | 2.32 | 501 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 2.74 | 0.94 | â | 1148 | â | 496 | â | 1(1) |
| Rain et al. | 2021 | 3.04 | 1.58 | â | 1445 | â | â | â | 4 |
| Dias et al. | 2021 | 2.67 | 1.92 | â | 1208 | -0.213 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.74 | 0.94 | â | 1148 | â | â | â | â |
| Kounkel et al. | 2020 | 2.84 | 2.13 | â | 407 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.04 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1180 | -0.250 | â | â | â |
| Monteiro & Dias | 2019 | 2.47 | 1.61 | â | 1466 | 0.021 | â | â | â |
| Soubiran et al. | 2018 | 3.04 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.04 | 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: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.90 (50th percentile), true positive (human-assigned).
Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.90 (50th percentile), true positive (human-assigned).
Rain et al. (2021)
This cluster was not include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl), parameters log(t)=9.16, E(b-v)=0.509 and Z=0.021 are from Monteiro & Dias (2019MNRAS.487.2385M).
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg40' along with Gulliver 3.