FSR 1407
(MWSC 1676; FoF 635)
0.89
UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad)
15.1 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1407 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very old cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 142.434 | -33.85 | 0.272 | -4.781 | 6.012 | 21.809 |
| Li et al. | 2025 | 142.445 | -33.848 | 0.275 | -4.806 | 5.983 | â |
| Hu & Soubiran | 2025 | 142.431 | -33.845 | â | â | â | â |
| Almeida et al. | 2025 | 142.455 | -33.851 | â | â | â | â |
| Hunt & Reffert | 2024 | 142.446 | -33.848 | 0.273 | -4.778 | 6.006 | 21.691 |
| Cavallo et al. | 2024 | 142.431 | -33.845 | 0.274 | â | â | â |
| Hunt & Reffert | 2023 | 142.446 | -33.848 | 0.273 | -4.778 | 6.006 | 21.691 |
| Just et al. | 2023 | 142.456 | -33.831 | â | â | â | â |
| Dias et al. | 2021 | 142.455 | -33.851 | 0.28 | -4.797 | 5.986 | 18.894 |
| Cantat-Gaudin et al. | 2020 | 142.445 | -33.848 | 0.275 | -4.806 | 5.983 | â |
| Cantat-Gaudin & Anders | 2020 | 142.445 | -33.848 | 0.275 | -4.806 | 5.983 | â |
| Liu & Pang | 2019 | 142.438 | -33.864 | 0.28 | -4.776 | 5.96 | â |
| Soubiran et al. | 2018 | 142.445 | -33.848 | â | â | â | 18.3 |
| Cantat-Gaudin et al. | 2018 | 142.445 | -33.848 | 0.275 | -4.806 | 5.983 | â |
| Kharchenko et al. | 2016 | 142.456 | -33.831 | â | â | â | â |
| Kharchenko et al. | 2013 | 142.462 | -33.835 | â | -11.96 | 8.89 | â |
| Froebrich et al. | 2007 | 142.442 | -33.831 | â | â | â | 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 | 3.29 | 0.405 | 1.02 | 5266 | -0.280 | 832 | â | â |
| Li et al. | 2025 | 3.35 | 0.36 | â | 7569 | -0.134 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.280(5) | â | â | â |
| Almeida et al. | 2025 | 3.16 | 0.33 | â | 8128 | â | 642 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 832(1) | â | â |
| Cavallo et al. | 2024 | 2.74 | 0.45 | â | 6457 | -0.370 | â | â | â |
| Hunt & Reffert | 2023 | 3.12 | 0.26 | 1.02 | 2704 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1995 | â | 2188 | â | â |
| Dias et al. | 2021 | 3.16 | 0.33 | â | 8128 | -0.138 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.45 | 0.57 | â | 4074 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.29 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 11500 | -1.750 | â | â | â |
| Soubiran et al. | 2018 | 3.29 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.29 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 3.86 | 0.64 | â | 1995 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.86 | 0.64 | â | 1995 | 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.