398182.fig.004a
(a)
398182.fig.004b
(b)
398182.fig.004c
(c)
398182.fig.004d
(d)
Figure 4: Three extracted CMDs for stars measured in the field of NGC 2107 distributed within the cluster radius (a), the cluster surrounding field for an equal cluster area (d), and the cluster cleaned from field contamination (c). The cluster radial profile is also depicted (b).