Gulliver 47
0.71
UTI
0.58
CN
0.83
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
6.7 [arcmin]
- CN 0.58 Moderately populated
- Cdens 0.83 Dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Gulliver 47 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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 metallicity parameter (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 107.927 | 0.82 | 0.49 | -1.928 | -0.448 | 47.047 |
| Li et al. | 2025 | 107.932 | 0.827 | 0.491 | -1.957 | -0.432 | â |
| Almeida et al. | 2025 | 107.919 | 0.841 | â | â | â | â |
| Zhang et al. | 2024 | 107.92 | 0.805 | â | â | â | â |
| Hunt & Reffert | 2024 | 107.92 | 0.805 | 0.47 | -1.896 | -0.48 | 45.942 |
| Cavallo et al. | 2024 | 107.928 | 0.811 | 0.473 | â | â | â |
| Hunt & Reffert | 2023 | 107.92 | 0.805 | 0.47 | -1.896 | -0.48 | 45.942 |
| Almeida et al. | 2023 | 107.91 | 0.837 | â | â | â | â |
| Dias et al. | 2021 | 107.919 | 0.841 | 0.49 | -1.97 | -0.435 | 47.521 |
| Cantat-Gaudin et al. | 2020 | 107.932 | 0.827 | 0.491 | -1.957 | -0.432 | â |
| Cantat-Gaudin & Anders | 2020 | 107.932 | 0.827 | 0.491 | -1.957 | -0.432 | â |
| Monteiro & Dias | 2019 | 107.932 | 0.827 | â | â | â | 2.401 |
| Cantat-Gaudin et al. | 2018 | 107.932 | 0.827 | 0.491 | -1.957 | -0.432 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.06 | 0.33 | â | 431 | 0.149 | â | â | â |
| Almeida et al. | 2025 | 1.82 | 0.54 | â | 373 | â | 278 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.029* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 431* | â | â |
| Cavallo et al. | 2024 | 1.94 | 0.30 | â | 457 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 1.90 | 0.19 | 0.77 | 518 | â | â | â | â |
| Almeida et al. | 2023 | 1.85 | 0.45 | â | 418 | -0.116 | 466* | 0.45 | â |
| Dias et al. | 2021 | 1.82 | 0.54 | â | 373 | -0.106 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.93 | 0.31 | â | 347 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.92 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 1.82 | 0.52 | â | 389 | 0.011 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.92 | â | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.