Table 5: Values for the reddening as determined in the present paper; the three E(B-V) values for each cluster derived from individual colours, i.e. from (B-V), (b-y), and (V-K) respectively, are also given. The last line gives the adopted reddening.
NGC 2506 NGC 6134 IC 4651

${\rm [Fe/H]}$ -0.20 +0.15 +0.11

$T_{\rm eff}$ (ref.) 5000 K 5000 K 4500 K

E(B-V)_BV $0.058\pm0.016$ $0.355\pm0.005$ $0.087\pm0.022$

$E(B-V)_{\rm by}$ $0.340\pm0.006$ $0.082\pm0.015$

E(B-V)_VK $0.076\pm0.007$ $0.388\pm0.005$ 0.080

E(B-V) adop. $0.073\pm0.009$ $0.363\pm0.014$ $0.083\pm0.011$

**Table 5:** Values for the reddening as determined in the present paper; the three E(B-V) values for each cluster derived from individual colours, i.e. from (B-V), (b-y), and (V-K) respectively, are also given. The last line gives the adopted reddening.
	NGC 2506	NGC 6134	IC 4651
${\rm [Fe/H]}$	-0.20	+0.15	+0.11
$T_{\rm eff}$ (ref.)	5000 K	5000 K	4500 K
E(B-V)_BV	$0.058\pm0.016$	$0.355\pm0.005$	$0.087\pm0.022$
$E(B-V)_{\rm by}$		$0.340\pm0.006$	$0.082\pm0.015$
E(B-V)_VK	$0.076\pm0.007$	$0.388\pm0.005$	0.080
E(B-V) adop.	$0.073\pm0.009$	$0.363\pm0.014$	$0.083\pm0.011$

Source LaTeX | All tables | In the text