the HST and Spitzer bands is slightly larger than expected. We consider that for the HST data the difference is attributed to our very large PSF correction factor applied to be matched with the Subaru images. For the Spitzer data the difference is due to the uncertainty in the aperture correction. We remark that our catalog tends to have the slightly bluer *K* $-$ \[3.6\] and *K* $-$ \[4.5\] colors than those of the published one.

 Example results of SED fitting  {#S2s3exs}
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We show two examples in figures \[fig2\] and \[fig3\] in order to show the validity of our SED fitting analysis. The first figure is the red LBG observed with Spitzer ($\beta_{\mathrm{obs}} = -1.27$ and $M_{\mathrm{UV,obs}} = -20.38$), and the second figure is the blue LBG observed without Spitzer ($\beta_{\mathrm{obs}} = -2.39$ and $M_{\mathrm{UV,obs}} = -20.32$). In the top nine panels of each figure, we show the stamps of the imaging data from Subaru/*B* to UKIRT/*K*. The center of the images represent the detected position, and the green two straight lines in each image with 1” length are placed at 1” from the detected position. In the bottom left panel, we show the observed photometry and best-fit SED. 