Updated calibrations for the hybrids tracers that combine FUV observed luminosity and IR luminosity. Top panels show the FUV_obs + 22 μm hybrid tracer, while the FUV_obs +TIR hybrid tracers appear on the bottom panels. Galaxies hosting type-2 AGN (orange points) are included on the left panels. Blue points refer to star-forming galaxies. Dashed lines correspond to the 1:1 line taking into account the C_Hα and C_FUV constants (5.5 × 10^-42 and 4.6 × 10^-44) given in Eqs. (3) and (4), respectively. The best-fitting a_IR coefficients calculated as the median value of the expression 17 are shown for clarity. These a_IR values and their corresponding errors appear in Table 3. The residuals are computed as the average value of the log[C_Hα × L [Hα_corr]/(C_FUV × (L [FUV_obs] + a_IR × L[IR]))], where L(IR) could be 22 μm or TIR, after applying a 4σ rejection. These hybrid tracers show a trend with the a_IR coefficient, so when type-2 AGN host galaxies are included the value of a_IR decreases.