Fig. 9From: Heliocentric distance dependence of zodiacal light observed by Hayabusa2#The sensitivity calibration. The linear relationship between the G-band flux of the selected stars and their detected signals in the W(x, y)/FLAT(x, y) image of the 2022–12-12 wide-band data as an example of the sensitivity calibration. The red line shows the best fit to the data, and the dashed lines show \(\pm 1\sigma\) deviationsBack to article page