LISC 3534
(OCSN 208)
0.51
UTI
0.85
CN
0.3
Cdens
1.0
CC3
0.19
Clit
1.0
Cdup
Nm (P>50%)
357
Core radius and density
5.3 [pc], 1.5 [pc-2]
- CN 0.85 Rich
- Cdens 0.3 Loose
- CC3 1.0 Very high quality
- Clit 0.19 Rarely studied
- Cdup 1.0 Unique
Overview
LISC 3534 is a rich, loose object of very high C3 quality. Its parallax locates it at a very close distance, below 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 rarely studied in the literature.
Note: This object shares a small 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 | 12.195 | 50.247 | 2.179 | 7.373 | -3.082 | -5.551 |
| Yan et al. | 2026 | 12.088 | 49.906 | 2.189 | 7.368 | -3.082 | â |
| Yang et al. | 2025 | 12.088 | 49.906 | â | â | â | â |
| Zhang et al. | 2024 | 12.088 | 49.906 | â | â | â | â |
| Hunt & Reffert | 2024 | 12.088 | 49.906 | 2.189 | 7.368 | -3.082 | -5.828 |
| Cavallo et al. | 2024 | 12.608 | 50.213 | 2.186 | â | â | â |
| Hunt & Reffert | 2023 | 12.088 | 49.906 | 2.189 | 7.368 | -3.082 | -5.828 |
| Qin et al. | 2023 | 11.97 | 50.3 | 2.18 | 7.39 | -3.1 | -5.02 |
| Li et al. | 2022 | 11.941 | 50.253 | 2.18 | 7.408 | -3.078 | 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 | 0.44 | 0.44 | 0.83 | 148 | -0.067 | 275 | 0.42 | â |
| Yan et al. | 2026 | â | â | â | 161 | â | â | â | â |
| Yang et al. | 2025 | â | â | â | 148 | -0.040(3) | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.093(1) | â | â | â |
| Hunt & Reffert | 2024 | 0.44 | 0.14 | 0.83 | 149 | â | 275(1) | â | â |
| Cavallo et al. | 2024 | 0.47 | 0.50 | â | 68 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.44 | 0.14 | 0.83 | 149 | â | â | â | â |
| Qin et al. | 2023 | 0.55 | 0.44 | â | 79 | â | â | â | â |
| Li et al. | 2022 | 0.41 | 0.59 | â | â | -0.279 | â | 0.42 | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Yan et al. (2026)
Number of WDs: expected from single-star evolution N=5, with probability of formation through binary evolution >=0.5 N=4.
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).