...z = 1.1

Full Table 2 is only available in electronic form at http://www.aanda.org

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... model

A star formation rate is proportional to $\exp~(-t/\tau)$.

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... performed

A significant fraction of galaxies at large radii is expected to be fore-/background galaxies, and the subtraction of them results in a large scatter with large errors in the data points. Thus, we do not subtract them and instead we draw the red fraction of the control field as the horizontal line.

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... sample

The $K_{\rm s}$-band characteristic magnitude of $z\sim1.1$ galaxies is $m_{K_{\rm s}}^*=20.5$(Strazzullo et al. 2006) and we reach $m_{K_{\rm s}}^*=22.9$ ( $=m_{K_{\rm s}}^*+2.4$) with the MOIRCS-shallow catalog. We applied the same magnitude cut relative to the characteristic magnitude to the sloan catalog.

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