Left: comparison of the IMFs below 1 M_⊙ in six different SFRs. The IMF for CrA is the mean of the IMFs presented in Section 4.3. The solid lines represent fits to the full set of data points for each cluster, and the dashed lines indicate fits restricted to the substellar regime below 0.2 M_⊙. Right: IMF slope α corresponding to the fits displayed in the left panel, indicated using matching line styles. Table 3 lists the values shown in this panel, along with the references.