Table 1: WEBDA parameters on well-studied open clusters.
Cluster [Fe/H] Age (Myr) $d_{\odot}$ (pc) $R_{\rm ex}$ ( $^\prime$ ) (m-M)_V (m-M)_J ( $m-M)_{K_{\rm S}}$ E(B-V) E(J-H) $E(J-K_{\rm S}$ )

Pleiades, M 45 +0.11 135 150 66 5.98 5.910 5.895 0.030 0.009 0.015

M 41, NGC 2287 +0.04 243 693 25 9.29 9.227 9.214 0.027 0.008 0.013

Praesepe, M 44, NGC 2632 +0.14 729 187 72 6.39 6.412 6.383 0.009 0.003 0.004

M 67, NGC 2682 -0.15 2564 908 15 9.98 9.799 9.794 0.059 0.018 0.029

NGC 6791 +0.11 4395 5853 7 14.21 13.936 13.879 0.117 0.036 0.057

**Table 1:** WEBDA parameters on well-studied open clusters.
Cluster	[Fe/H]	Age (Myr)	$d_{\odot}$ (pc)	$R_{\rm ex}$ ( $^\prime$ )	(m-M)_V	(m-M)_J	( $m-M)_{K_{\rm S}}$	E(B-V)	E(J-H)	$E(J-K_{\rm S}$ )
Pleiades, M 45	+0.11	135	150	66	5.98	5.910	5.895	0.030	0.009	0.015
M 41, NGC 2287	+0.04	243	693	25	9.29	9.227	9.214	0.027	0.008	0.013
Praesepe, M 44, NGC 2632	+0.14	729	187	72	6.39	6.412	6.383	0.009	0.003	0.004
M 67, NGC 2682	-0.15	2564	908	15	9.98	9.799	9.794	0.059	0.018	0.029
NGC 6791	+0.11	4395	5853	7	14.21	13.936	13.879	0.117	0.036	0.057

Column 4: distance to the Sun; Col. 5: radius used for VizieR extraction.

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