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$K'$-band imaging observations were performed on 2000 November 17 and 18, and $J$-band imaging observation was made on 2002 January 6, using the Cooled Infrared Spectrograph and Camera for OHS(CISCO)(Motohara et al. 2002) attached to the Nasmyth focus of Subaru Telescope. Both clusters’ images were taken by using 8 points dithering of 12 exposures with 20 s each for the $K'$-band and of 6 exposures with 40 s for the $J$-band, covering about a 2.0$\times$2.0 field of view. The total exposure times were 9220 s in the $K'$-band, and 3600 s in the $J$-band for MS $0451.6-0305$ and 6880 s in the $K'$-band for MS $0440.5+0204$. The seeing sizes were 0.6 to 0.8 in the $K'$-band, and 0.7 to 0.9 in the $J$-band. The sky conditions were mostly photometric during the observation in 2000 November, but not on 2002 January 6. We used FS10 and FS12 from the UKIRT faint standard catalog (Casali & Hawarden 1992) for photometric calibrations. The depth of our observations reached to 22.1 mag in $K'$ and 22.3 mag in $J$ with 1$\sigma$ detection within 2” diameter. For $K'$, we estimated the errors in our photometry to be less than 0.1 magnitude, but we could 