Table 1.
Stars observed, open cluster membership, and instrumental setup.
| Star | G/Ks | Type | Cluster | p | DR3 parallax | Instrument |
|---|---|---|---|---|---|---|
| (mag) | (mas) | |||||
| Case 63 | 11.5/3.6 | C | Berkeley 9 | 0.99 | 0.573±0.031 | TNG-GIARPS |
| HD 292921 | 10.4/6.0 | M | Berkeley 34 | 0.99 | 0.246±0.020 | CAHA-CARMENES |
| IRAS 20540+5049★ | 12.6/5.0 | M | Berkeley 53 | 0.99 | 0.355±0.049 | TNG-GIARPS |
| Case 473 | 11.9/4.9 | C | Berkeley 53 | 0.68 | 0.274±0.033 | TNG-GIARPS |
| 2MASS J20560894+5059071★ | 12.5/5.8 | M | Berkeley 53 | 0.99 | 0.344±0.045 | CAHA-CARMENES |
| Case 121 | 10.7/4.9 | C | Berkeley 72 | 0.99 | 0.198±0.034 | TNG-GIARPS |
| CAHA-CARMENES | ||||||
| Case 588 | 10.6/4.9 | C | Dias 2 | 0.99 | 0.214±0.034 | CAHA-CARMENES |
| DH Mon | 10.8/5.0 | C | Dias 2 | 0.68 | 0.266±0.037 | CAHA-CARMEES |
| IRAS 19582+2907 | 13.4/5.2 | C | FSR 0172 | 0.99 | 0.202±0.052 | CAHA-CARMENES |
| HD 11800 | 9.6/3.2 | K | NGC 743 | 0.68 | 0.876±0.016 | CAHA-CARMENES |
| TNG-GIARPS | ||||||
| [D75b] Star30 | 11.1/6.0 | MS | NGC 1798 | 0.99 | 0.291±0.031 | CAHA-CARMENES |
| BD +60 2534 | 8.2/4.2 | K | NGC 7654 | 0.99 | 0.628±0.016 | CAHA-CARMENES |
| TNG-GIARPS | ||||||
| MSB 75 | 10.7/3.1 | C | NGC 7789 | 0.99 | 0.478±0.025 | TNG-GIARPS |
| C* 908 | 10.2/5.1 | C | Ruprecht 37 | 0.99 | 0.261±0.024 | CAHA-CARMENES |
| CSS 0291 | 10.3/4.2 | S | Tombaugh 1 | 0.99 | 0.418±0.024 | CAHA-CARMENES |
| V493 Mon | 12.3/4.9 | C | Trumpler 5 | 0.68 | 0.368±0.036 | CAHA-CARMENES |
Notes. p is the membership probability according to the analysis by Marigo et al. (2022) and Cantat-Gaudin & Anders (2020) (see text). The spectral types were taken from SIMBAD: https://simbad.unistra.fr/simbad/. The two stars marked with ★ appear in SIMBAD with an unknown spectral type. However, from their high resolution spectra obtained here we classified them as typical M-stars.
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