Table 6.
Open in new tab

The colour-excess ratios in different filters for each cluster. The normal values are taken from Dutra et al. (2002); Dias et al. (2012); Wang & Chen (2019).

Cluster|$\frac{E(B-V)}{E(G_{\rm BP}-G_{\rm RP})}$||$\frac{E(V-I)}{E(B-V)}$||$\frac{E(J-H)}{E(B-V)}$||$\frac{E(J-K_{s})}{E(B-V)}$|
(mag)(mag)(mag)(mag)
Normal0.761.250.330.49
NGC 11930.62 ± 0.101.25 ± 0.05––
NGC 23550.65 ± 0.121.33 ± 0.110.330.50 ± 0.10
King 120.66 ± 0.031.29 ± 0.030.34 ± 0.020.50 ± 0.02
Cluster|$\frac{E(B-V)}{E(G_{\rm BP}-G_{\rm RP})}$||$\frac{E(V-I)}{E(B-V)}$||$\frac{E(J-H)}{E(B-V)}$||$\frac{E(J-K_{s})}{E(B-V)}$|
(mag)(mag)(mag)(mag)
Normal0.761.250.330.49
NGC 11930.62 ± 0.101.25 ± 0.05––
NGC 23550.65 ± 0.121.33 ± 0.110.330.50 ± 0.10
King 120.66 ± 0.031.29 ± 0.030.34 ± 0.020.50 ± 0.02
Table 6.
Open in new tab

The colour-excess ratios in different filters for each cluster. The normal values are taken from Dutra et al. (2002); Dias et al. (2012); Wang & Chen (2019).

Cluster|$\frac{E(B-V)}{E(G_{\rm BP}-G_{\rm RP})}$||$\frac{E(V-I)}{E(B-V)}$||$\frac{E(J-H)}{E(B-V)}$||$\frac{E(J-K_{s})}{E(B-V)}$|
(mag)(mag)(mag)(mag)
Normal0.761.250.330.49
NGC 11930.62 ± 0.101.25 ± 0.05––
NGC 23550.65 ± 0.121.33 ± 0.110.330.50 ± 0.10
King 120.66 ± 0.031.29 ± 0.030.34 ± 0.020.50 ± 0.02
Cluster|$\frac{E(B-V)}{E(G_{\rm BP}-G_{\rm RP})}$||$\frac{E(V-I)}{E(B-V)}$||$\frac{E(J-H)}{E(B-V)}$||$\frac{E(J-K_{s})}{E(B-V)}$|
(mag)(mag)(mag)(mag)
Normal0.761.250.330.49
NGC 11930.62 ± 0.101.25 ± 0.05––
NGC 23550.65 ± 0.121.33 ± 0.110.330.50 ± 0.10
King 120.66 ± 0.031.29 ± 0.030.34 ± 0.020.50 ± 0.02
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