We present 31.5 \mu m imaging photometry of 11 nearby Seyfert galaxies observed from the Stratospheric Observatory For Infrared Astronomy ( SOFIA ) using the Faint Object infraRed CAmera for the SOFIA Telescope ( FORCAST ) .
We tentatively detect extended 31 \mu m emission for the first time in our sample .
In combination with this new data set , subarcsecond resolution 1 - 18 \mu m imaging and 7.5 - 13 \mu m spectroscopic observations were used to compute the nuclear spectral energy distribution ( SED ) of each galaxy .
We found that the turnover of the torus emission does not occur at wavelengths \leq 31.5 \mu m , which we interpret as a lower-limit for the wavelength of peak emission .
We used Clumpy torus models to fit the nuclear infrared ( IR ) SED and infer trends in the physical parameters of the AGN torus for the galaxies in the sample .
Including the 31.5 \mu m nuclear flux in the SED 1 ) reduces the number of clumpy torus models compatible with the data , and 2 ) modifies the model output for the outer radial extent of the torus for 10 of the 11 objects .
Specifically , six ( 60 % ) objects show a decrease in radial extent while four ( 40 % ) show an increase .
We find torus outer radii ranging from < 1pc to 8.4 pc .