Juchert Saloran 1
(Juchert-Saloranta 1; MWSC 28; DSH J0016.3+5957; FSR 0478)
0.95
UTI
0.75
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
13.5 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Juchert Saloran 1 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a moderate 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 | 4.078 | 59.962 | 0.178 | -1.643 | -1.282 | -81.792 |
| Li et al. | 2025 | 4.078 | 59.967 | 0.197 | -1.731 | -1.312 | â |
| Hu & Soubiran | 2025 | 4.072 | 59.965 | â | â | â | â |
| Almeida et al. | 2025 | 4.074 | 59.967 | â | â | â | â |
| Hunt & Reffert | 2024 | 4.081 | 59.965 | 0.183 | -1.642 | -1.298 | â |
| Cavallo et al. | 2024 | 4.072 | 59.965 | 0.18 | â | â | â |
| Hunt & Reffert | 2023 | 4.081 | 59.965 | 0.183 | -1.642 | -1.298 | â |
| Just et al. | 2023 | 4.072 | 59.959 | â | â | â | â |
| Dias et al. | 2021 | 4.074 | 59.967 | 0.165 | -1.69 | -1.297 | -76.907 |
| Cantat-Gaudin et al. | 2020 | 4.078 | 59.967 | 0.197 | -1.731 | -1.312 | â |
| Cantat-Gaudin & Anders | 2020 | 4.078 | 59.967 | 0.197 | -1.731 | -1.312 | â |
| Soubiran et al. | 2018 | 4.078 | 59.967 | â | â | â | -77.85 |
| Bica et al. | 2019 | 4.089 | 59.963 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.078 | 59.967 | 0.197 | -1.731 | -1.312 | â |
| Loktin & Popova | 2017 | 4.08 | 59.962 | â | -0.81 | -3.442 | â |
| Kharchenko et al. | 2016 | 4.072 | 59.959 | â | â | â | â |
| Dias et al. | 2014 | 4.083 | 59.962 | â | -0.59 | 0.58 | â |
| Kharchenko et al. | 2013 | 4.081 | 59.962 | â | -2.38 | -1.24 | â |
| Kharchenko et al. | 2012 | 4.081 | 59.962 | â | -2.42 | -1.19 | â |
| Kronberger et al. | 2006 | 4.085 | 59.962 | â | â | â | â |
| Dias et al. | 2002 | 4.083 | 59.962 | â | -0.59 | 0.58 | 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 | 4.84 | 2.58 | 1.93 | 992 | -0.006 | 1188 | â | â |
| Li et al. | 2025 | 5.54 | 2.99 | â | 861 | 0.089 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.390(5) | â | â | â |
| Almeida et al. | 2025 | 5.15 | 2.92 | â | 638 | â | 1192 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1188(1) | â | â |
| Cavallo et al. | 2024 | 4.53 | 2.51 | â | 759 | 0.450 | â | â | â |
| Hunt & Reffert | 2023 | 4.30 | 2.81 | 1.93 | 375 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1995 | â | 1026 | â | â |
| Dias et al. | 2021 | 5.15 | 2.92 | â | 638 | -0.101 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 5.40 | 2.82 | â | 603 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.43 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.43 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.43 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.19 | 1.96 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2016 | 5.33 | 2.58 | â | 1995 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.33 | 2.58 | â | 1995 | â | â | â | â |
| Kharchenko et al. | 2012 | 5.33 | 2.58 | â | 1995 | â | â | â | â |
| Dias et al. | 2002 | 3.86 | 2.57 | â | 1122 | 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: intermediate fit.
Cavallo et al. (2024)
Gold sample.