Kennicutt–Schmidt diagram of BX610 for 0.18″ overlapped apertures of the center (crosses), the clump (stars), and the disk (circles). SFR values for disk and clump regions are derived from extinction-corrected Hα flux, while for central regions, they are based on dust continuum emission. The color bar indicates the distance to the center as a function of the stellar effective radius. A typical error bar is shown in the bottom right corner. The dotted diagonal lines correspond to constant gas depletion times of 0.1, 1, and 10 Gyr from top to bottom. The red dashed line correspond to the ordinary least-squares bisector fit for all data points. The gray data points from Genzel et al. (2010) and Tacconi et al. (2013) are indicated for comparison with whole galaxies, while the data points from Freundlich et al. (2013) are for spatially resolved main-sequence galaxies at z ∼ 1.