Fig. 9
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Application of the PDR pack to the obscured AGN of VV114. The corresponding apertures are analogous to Donnan et al. (2024). The displayed τ9.7 are those resulting from PAHFIT, while Donnan et al. (2024) report total optical depths (τ9.8) of the order 1 and 5 for VV114 SW and NE respectively. Due to the limitations at higher dust attenuation, the 7.7 and 13.3 μm broad components are likely overestimated for VV114 NE, while the mismatch near 15 μm becomes larger.
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