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We report near simultaneous imaging using LMIRCam on the LBTI of thequadruply imaged lensed quasar HS 0810+2554 at wavelengths of 2.16, 3.7 and$4.78~\mu$m with a Full Width Half Max (FWHM) spatial resolution of$0^{\prime\prime}\!\!.13$, $0^{\prime\prime}\!\!.12$ and$0^{\prime\prime}\!\!.15$ respectively, comparable to HST optical imaging. Inthe $\rm{z} = 1.5$ rest frame of the quasar, the observed wavelengthscorrespond to 0.86, 1.48, and $1.91~\mu$m respectively. The two brightestimages in the quad, A and B, are clearly resolved from each other with aseparation of $0.187^{\prime\prime}$. The flux ratio of these two images (A/B)trends from 1.79 to 1.23 from 2.16 to $4.78~\mu$m. The trend in flux ratio isconsistent with the $2.16~\mu$m flux originating from a small sized accretiondisk in the quasar that experiences only microlensing. The excess flux abovethe contribution from the accretion disk at the two longer wavelengthsoriginates from a larger sized region that experiences no microlensing. Asimple model employing multiplicative factors for image B due to stellarmicrolensing $(m)$ and sub-structure millilensing $(M)$ is presented. Theresult is tightly constrained to the product $m\times M=1.79$. Given theobservational errors, the 60\% probability contour for this product stretchesfrom $m= 2.6$, $M = 0.69$ to $m= 1.79$, $M = 1.0$, where the later isconsistent with microlensing only.

Image Flux Ratios of Gravitationally Lensed HS 0810+2554 with High Resolution Infrared Imaging