Table 3
Extinction, reddening, distance modulus, and distances for the clusters.
| Nataf method | ||||||
|---|---|---|---|---|---|---|
| Name | AV | E(B-V) | AKs | E(J-Ks) | (m-M)0 | D (kpc) |
| BH118 | 1.66±0.10 | 0.53 ± 0.05 | 0.12 ± 0.01 | 0.05 ± 0.00 | 14.57 ± 0.02 | 8.18 ± 0.07 |
| BH144 | 2.52 ± 0.10 | 0.81 ± 0.06 | 0.19 ± 0.01 | 0.08 ± 0.00 | 14.64 ± 0.04 | 8.51 ± 0.16 |
| Schuster-MWSC1756 | 10.76 ± 0.10 | 3.47 ± 0.20 | 0.80 ± 0.01 | 0.34 ± 0.01 | 14.06 ± 0.03 | 6.49 ± 0.10 |
| Saurer 3 | 2.56 ± 0.10 | 0.83 ± 0.06 | 0.19 ± 0.01 | 0.08 ± 0.00 | 14.28 ± 0.03 | 7.16 ± 0.09 |
| FSR1521 | 10.32 ± 0.10 | 3.33 ± 0.20 | 0.77 ± 0.01 | 0.33 ± 0.01 | 12.45 ± 0.02 | 3.09 ± 0.03 |
| Saurer 2 | 5.85 ± 0.10 | 1.89 ± 0.11 | 0.43 ± 0.01 | 0.19 ± 0.04 | 13.56 ± 0.04 | 5.14 ± 0.09 |
| Haffner10-FSR1231 | 2.05 ± 0.10 | 0.66 ± 0.05 | 0.15 ± 0.01 | 0.07 ± 0.00 | 12.66 ± 0.04 | 3.62 ± 0.07 |
| Jurchert12 | 2.60 ± 0.10 | 0.84 ± 0.06 | 0.19 ± 0.01 | 0.08 ± 0.00 | 14.69 ± 0.02 | 8.84 ± 0.07 |
| Pismis3 | 4.37 ± 0.10 | 1.41 ± 0.09 | 0.33 ± 0.09 | 0.14 ± 0.04 | 11.72 ± 0.07 | 2.20 ± 0.07 |
| Ruiz–Dern method | ||||||
| BH118 | 0.07 ± 0.03 | 0.16 ± 0.03 | 14.61 ± 0.03 | 8.36 ± 0.03 | ||
| BH144 | 0.07 ± 0.08 | 0.17 ± 0.08 | 14.76 ± 0.11 | 8.95 ± 0.11 | ||
| Schuster-MWSC1756 | 0.57 ± 0.04 | 1.34 ± 0.04 | 14.29 ± 0.05 | 7.21 ± 0.05 | ||
| Saurer 3 | 0.16 ± 0.03 | 0.37 ± 0.03 | 14.30 ± 0.04 | 7.25 ± 0.04 | ||
| FSR1521 | 0.62 ± 0.05 | 1.44 ± 0.05 | 12.59 ± 0.10 | 3.31 ± 0.10 | ||
| Saurer 2 | 0.26 ± 0.03 | 0.60 ± 0.03 | 13.74 ± 0.05 | 5.59 ± 0.05 | ||
| Haffner10-FSR1231 | − | − | − | − | − | − |
| Jurchert12 | 0.11 ± 0.07 | 0.26 ± 0.07 | 14.77 ± 0.07 | 8.97 ± 0.07 | ||
| Pismis3 | 0.19 ± 0.08 | 0.44 ± 0.08 | 11.71 ± 0.10 | 2.19 ± 0.10 | ||
Notes. The Nataf method derives from the relation presented in Nataf et al. (2015). However, we obtained the AV values from the NASA/IPAC Infrared Science Archive (https://irsa.ipac.caltech.edu/applications/DUST/), which uses the extinction maps from Schlafly & Finkbeiner (2011) and Schlegel et al. (1998) to compute AV for a given source. For our analysis, we adopted the values provided by SF11. It is important to note that the errors in AKs and E(J-Ks) are not zero. When rounded to three decimal places, the values are AKs = [0.008, 0.008, 0.013, 0.008, 0.013, 0.010, 0.010, 0.086] and E(J-Ks) = [0.003, 0.003, 0.006, 0.003, 0.006, 0.041, 0.003, 0.003, 0.037.]
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