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Table 3:

Newly derived masses and dissolution times for the studied clusters.

Name 		$\alpha_{J2000}$ $\delta_{J2000}$ J H K $\log$ Mass $\varepsilon$log Mass $t_{\rm diss}^{\rm Pap-III}$
            ($M_{\odot}$) ($M_{\odot}$) (Myr)

B015D-D041 		  $00^{\rm h}$ $41^{\rm m}$ $02.74^{\rm s}$ $+41\hbox{$^\circ$ }$ $06\hbox{$^\prime$ }$ $36.63\hbox{$^{\prime\prime}$ }$ 17.03 $\pm $ 0.42 15.37 $\pm $ 0.27 14.89 $\pm $ 0.25 4.2 0.09 112
B040-G102   $00^{\rm h}$ $41^{\rm m}$ $38.90^{\rm s}$ $+40\hbox{$^\circ$ }$ $40\hbox{$^\prime$ }$ $54.15\hbox{$^{\prime\prime}$ }$ 15.48 $\pm $ 0.08 14.90 $\pm $ 0.19 14.50 $\pm $ 0.15 4.6 0.07 631
B043-G106 $00^{\rm h}$ $41^{\rm m}$ $42.31^{\rm s}$ $+40\hbox{$^\circ$ }$ $42\hbox{$^\prime$ }$ $39.86\hbox{$^{\prime\prime}$ }$ 15.58 $\pm $ 0.07 15.50 $\pm $ 0.31 15.08 $\pm $ 1.00 4.4 0.10 3467
B066-G128 $00^{\rm h}$ $42^{\rm m}$ $03.14^{\rm s}$ $+40\hbox{$^\circ$ }$ $44\hbox{$^\prime$ }$ $48.55\hbox{$^{\prime\prime}$ }$ 16.25 $\pm $ 0.19 15.81 $\pm $ 0.47 16.06 $\pm $ 1.00 4.2 0.08 891
B081-G142 $00^{\rm h}$ $42^{\rm m}$ $13.59^{\rm s}$ $+40\hbox{$^\circ$ }$ $48\hbox{$^\prime$ }$ $38.96\hbox{$^{\prime\prime}$ }$ 14.55 $\pm $ 0.05 13.77 $\pm $ 0.07 13.76 $\pm $ 0.06 5.1 0.04 955
B257D-D073 $00^{\rm h}$ $44^{\rm m}$ $59.35^{\rm s}$ $+41\hbox{$^\circ$ }$ $54\hbox{$^\prime$ }$ $47.47\hbox{$^{\prime\prime}$ }$ 15.28 $\pm $ 0.10 14.77 $\pm $ 0.20 15.53 $\pm $ 1.00 4.6 0.09 302
B318-G042 $00^{\rm h}$ $40^{\rm m}$ $00.80^{\rm s}$ $+40\hbox{$^\circ$ }$ $34\hbox{$^\prime$ }$ $09.06\hbox{$^{\prime\prime}$ }$ 16.17 $\pm $ 1.00 16.39 $\pm $ 0.66 15.49 $\pm $ 1.00 3.8 0.29 1905
B321-G046 $00^{\rm h}$ $40^{\rm m}$ $15.33^{\rm s}$ $+40\hbox{$^\circ$ }$ $27\hbox{$^\prime$ }$ $45.98\hbox{$^{\prime\prime}$ }$ 17.11 $\pm $ 0.45 15.88 $\pm $ 0.57 15.18 $\pm $ 0.29 4.2 0.13 200
B327-G053   $00^{\rm h}$ $40^{\rm m}$ $24.12^{\rm s}$ $+40\hbox{$^\circ$ }$ $36\hbox{$^\prime$ }$ $22.38\hbox{$^{\prime\prime}$ }$ 14.91 $\pm $ 0.07 14.32 $\pm $ 0.10 14.14 $\pm $ 0.15 4.5 0.06 2754
B376-G309   $00^{\rm h}$ $45^{\rm m}$ $48.38^{\rm s}$ $+41\hbox{$^\circ$ }$ $42\hbox{$^\prime$ }$ $39.87\hbox{$^{\prime\prime}$ }$ 16.59 $\pm $ 0.18 16.07 $\pm $ 0.80 16.02 $\pm $ 1.00 4.1 0.09 295
B448-D035   $00^{\rm h}$ $40^{\rm m}$ $36.52^{\rm s}$ $+40\hbox{$^\circ$ }$ $40\hbox{$^\prime$ }$ $14.94\hbox{$^{\prime\prime}$ }$ 16.51 $\pm $ 0.34 16.45 $\pm $ 1.00 15.66 $\pm $ 1.22 4.1 0.16 115
B475-V128   $00^{\rm h}$ $44^{\rm m}$ $55.92^{\rm s}$ $+41\hbox{$^\circ$ }$ $54\hbox{$^\prime$ }$ $00.33\hbox{$^{\prime\prime}$ }$ 15.10 $\pm $ 0.08 14.68 $\pm $ 0.12 14.38 $\pm $ 0.17 4.7 0.07 1445
V031   $00^{\rm h}$ $41^{\rm m}$ $12.17^{\rm s}$ $+41\hbox{$^\circ$ }$ $05\hbox{$^\prime$ }$ $30.21\hbox{$^{\prime\prime}$ }$ 14.80 $\pm $ 0.06 14.42 $\pm $ 1.00 13.77 $\pm $ 0.11 4.8 0.10 1230
B083-G146   $00^{\rm h}$ $42^{\rm m}$ $16.46^{\rm s}$ $+41\hbox{$^\circ$ }$ $45\hbox{$^\prime$ }$ $20.53\hbox{$^{\prime\prime}$ }$ 14.88 $\pm $ 0.05 14.62 $\pm $ 0.12 14.07 $\pm $ 0.13 >4.7 $\dots$ $\dots$
B222-G277 $00^{\rm h}$ $44^{\rm m}$ $25.29^{\rm s}$ $+41\hbox{$^\circ$ }$ $14\hbox{$^\prime$ }$ $11.62\hbox{$^{\prime\prime}$ }$ 15.27 $\pm $ 0.13 14.41 $\pm $ 0.09 14.16 $\pm $ 0.08 >4.6 $\dots$ $\dots$
B347-G154 $00^{\rm h}$ $42^{\rm m}$ $22.89^{\rm s}$ $+41\hbox{$^\circ$ }$ $54\hbox{$^\prime$ }$ $27.40\hbox{$^{\prime\prime}$ }$ 14.68 $\pm $ 0.05 14.17 $\pm $ 0.04 14.17 $\pm $ 0.18 >4.7 $\dots$ $\dots$
B374-G306 $00^{\rm h}$ $45^{\rm m}$ $44.53^{\rm s}$ $+41\hbox{$^\circ$ }$ $41\hbox{$^\prime$ }$ $55.10\hbox{$^{\prime\prime}$ }$ 17.21 $\pm $ 0.50 18.50 $\pm $ 0.82 16.32 $\pm $ 0.84 >3.9 $\dots$ $\dots$
NB16 $00^{\rm h}$ $42^{\rm m}$ $33.11^{\rm s}$ $+41\hbox{$^\circ$ }$ $20\hbox{$^\prime$ }$ $16.48\hbox{$^{\prime\prime}$ }$ 14.91 $\pm $ 0.09 14.11 $\pm $ 0.07 13.46 $\pm $ 0.11 >4.8 $\dots$ $\dots$
P09b                
B049-G112 $00^{\rm h}$ $41^{\rm m}$ $45.59^{\rm s}$ $+40\hbox{$^\circ$ }$ $49\hbox{$^\prime$ }$ $54.53\hbox{$^{\prime\prime}$ }$ 15.53 $\pm $ 0.13 15.27 $\pm $ 0.23 14.42 $\pm $ 0.06 4.5 0.09 $\dots$
B367-G292 $\dots$ $\dots$ $\dots$ $\dots$ $\dots$ [4.3]a [0.11] $\dots$
B458-D049 $00^{\rm h}$ $41^{\rm m}$ $44.60^{\rm s}$ $+40\hbox{$^\circ$ }$ $51\hbox{$^\prime$ }$ $20.40\hbox{$^{\prime\prime}$ }$ 16.69 $\pm $ 0.35 15.04 $\pm $ 0.15 14.96 $\pm $ 0.15 4.1 0.15 $\dots$
B521 $00^{\rm h}$ $41^{\rm m}$ $41.80^{\rm s}$ $+40\hbox{$^\circ$ }$ $52\hbox{$^\prime$ }$ $02.41\hbox{$^{\prime\prime}$ }$ 17.32 $\pm $ 0.51 16.27 $\pm $ 0.43 16.28 $\pm $ 0.60 3.9 0.16 $\dots$
M039 $\dots$ $\dots$ $\dots$ $\dots$ $\dots$ [3.8]a [0.16] $\dots$
M050 $00^{\rm h}$ $44^{\rm m}$ $40.83^{\rm s}$ $+41\hbox{$^\circ$ }$ $30\hbox{$^\prime$ }$ $09.68\hbox{$^{\prime\prime}$ }$ 16.14 $\pm $ 0.14 14.90 $\pm $ 0.19 15.01 $\pm $ 0.31 4.3 0.13 $\dots$
WH01                
B315-G038 $00^{\rm h}$ $39^{\rm m}$ $48.51^{\rm s}$ $+40\hbox{$^\circ$ }$ $31\hbox{$^\prime$ }$ $30.33\hbox{$^{\prime\prime}$ }$ 14.99 $\pm $ 0.09 14.49 $\pm $ 0.10 14.24 $\pm $ 0.09 4.6 0.05 4074
B319-G044 $00^{\rm h}$ $40^{\rm m}$ $03.03^{\rm s}$ $+40\hbox{$^\circ$ }$ $33\hbox{$^\prime$ }$ $58.25\hbox{$^{\prime\prime}$ }$ 16.30 $\pm $ 0.12 15.94 $\pm $ 0.47 16.78 $\pm $ 0.52 3.9 0.10 182
B342-G094 $00^{\rm h}$ $41^{\rm m}$ $24.15^{\rm s}$ $+40\hbox{$^\circ$ }$ $36\hbox{$^\prime$ }$ $48.55\hbox{$^{\prime\prime}$ }$ 16.67 $\pm $ 0.48 15.57 $\pm $ 0.38 16.94 $\pm $ 1.00 4.0 0.17 214
B368-G293 $00^{\rm h}$ $44^{\rm m}$ $47.50^{\rm s}$ $+41\hbox{$^\circ$ }$ $51\hbox{$^\prime$ }$ $09.39\hbox{$^{\prime\prime}$ }$ 15.89 $\pm $ 0.27 15.14 $\pm $ 0.35 14.60 $\pm $ 0.21 4.4 0.08 251

Notes. In a few cases the data allowed us to obtain only a lower limit to the mass. $\alpha_{J2000}$ and $\delta_{J2000}$ are from 2MASS-6X-PSC catalog, J, H, K are from r = 10 $.\!\!^{\prime\prime}$0 ap. phot. in the 2MASS-6X-PSC catalog. Note that errJHK = 1.00 corresponds to errJHK=null in the 2MASS-6X-PSC catalog. (a) Estimated from Fig. 14, as these clusters lack NIR photometry. These mass estimates will not be used in the following to preserve the homogeneity of the sample.


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