Table A.2:
Reddening values for the five clusters compared to recent
literature papers.
| Cluster |
E(B-V) |
Literature |
| |
(rms) |
|
| NGC 2660 |
0.433 |
0.40 
0.02 (S, Z=0.02) |
| |
(0.020) |
0.37
0.02 (Tw, [Fe/H] = -0.18) |
| NGC 3960 |
0.294 |
0.29 (P, Z=0.01, diff.) |
| |
(0.043) |
0.29
0.02 (B, Z= 0.01-0.02, diff.) |
| |
|
0.33 (M) |
| |
|
0.30
0.01 (Tw, Fe/H] = -0.17) |
| Berkeley 32 |
0.139 |
0.10 (D, Z=0.008) |
| |
(0.017) |
0.10 (H, Z=0.008) |
| |
|
0.16 (KM, [Fe/H] = -0.4) |
| |
|
0.08 (R, [Fe/H] = -0.2) |
| |
|
0.12 (T, Z=0.008) |
| NGC 2324 |
0.193 |
0.17 (Ky, [Fe/H] = -0.3) |
| |
(0.016) |
0.25 (Pi, [Fe/H] = -0.31) |
| NGC 2477 |
0.299 |
0.2-0.4 (K, [Fe/H] = -0.05) |
| |
(0.025) |
|