Table 2.
Open cluster parameters based on the recent bibliography.
| Cluster | Cantat-Gaudin et al. (2020) | Hunt & Reffert (2023) | Cavallo et al. (2024) | ||||||
|---|---|---|---|---|---|---|---|---|---|
| AV | D | log (age) | AV | D | log (age) | AV | D | log (age) | |
| (mag) | (pc) | (a) | (mag) | (pc) | (a) | (mag) | (pc) | (a) | |
| Berkeley 9 | 2.69 | 1814 | 9.14 | 3.04 | 1690 | 8.93 | 3.06 | 1713 | 9.18 |
| Berkeley 34 | 1.64 | 7609 | 9.38 | 1.38 | 5051 | 8.28 | 1.80 | 4808 | 8.74 |
| Berkeley 53 | 4.42 | 3415 | 8.99 | 5.46 | 3407 | 8.75 | 4.97 | 4073 | 8.65 |
| Berkeley 72 | 1.65 | 5482 | 7.73 | 1.88 | 5076 | 8.47 | 1.77 | 5807 | 8.71 |
| Dias 2 | 0.47 | 4009 | 9.24 | 0.34 | 3897 | 9.21 | 1.72 | 3630 | 8.76 |
| FSR 0172 | 4.10 | 2979 | 8.20 | 5.20 | 3058 | 7.73 | 4.85 | 3801 | 8.96 |
| NGC 743 | 1.40 | 1168 | 8.00 | 1.47 | 1058 | 7.75 | 1.79 | 1164 | 7.55 |
| NGC 1798 | 1.12 | 5124 | 9.22 | 1.47 | 4167 | 8.96 | 1.63 | 3908 | 9.19 |
| NGC 7654 | 1.85 | 1653 | 8.19 | 1.94 | 1570 | 7.92 | 1.99 | 1698 | 8.16 |
| NGC 7789 | 0.83 | 2074 | 9.19 | 0.79 | 1968 | 9.19 | 1.03 | 1976 | 9.13 |
| Ruprecht 37 | 0.96 | 4526 | 9.35 | 0.23 | 4598 | 9.21 | 1.01 | 3548 | 9.53 |
| Tombaugh 1 | 0.66 | 2554 | 9.10 | 0.40 | 2323 | 9.09 | 0.71 | 2322 | 9.14 |
| Trumpler 5 | 1.20 | 3047 | 9.63 | 1.73 | 2904 | 9.33 | 1.79 | 2937 | 9.52 |
Notes. Extinction, distance, and age shown are the median values derived for each cluster by the corresponding authors. Cantat-Gaudin & Anders (2020) do not show uncertainties in their catalogue. The 16th and 84th quantiles of the corresponding distributions of the extinction, distance, and age obtained by Hunt & Reffert (2023) and Cavallo et al. (2024) vary typically respect to the median value in: ±30%, ±2%, ±5%, and ±10%, ±16%, and ±2%, respectively.
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