Fig. 4From: Heliocentric distance dependence of zodiacal light observed by Hayabusa2#Dataset acquired for one ZL observation. One dataset includes one bias image B(x, y), three wide-band images \(W_i(x,y)\) (\(i=\)1-3), two v-band images \(V_j(x,y)\) (\(j=\)1-2), and their respective optical-black images (Bb(x, y), \(Wb_i(x,y)\), and \(Vb_j(x,y)\))Back to article page