L_{IR,24   μm}/L_IR,PACS ratio versus L_{IR,24   μm} obtained using the CE01 method, in the left panel. L_{IR,24   μm}/L_IR,PACS ratio versus the M/M_⊙ using the CE01 method, in the central panel. L_{IR,24   μm}/L_IR,PACS ratio versus the L_{IR,24   μm} obtained using the R10 method, in the right panel. In all panels empty circles are normal star forming galaxies in our sample with both a MIPS 24 μm and PACS 100 or 160 μm detection. Filled points are low luminosity obscured AGNs with both a MIPS 24 μm and PACS 100 or 160 μm detection. The point with error bar is the result of the stacking analysis in the GOODS-N 160 μm map of the obscured AGNs of our sample with only MIPS detection.