SiO maser emissions integrated over V_LSR from −28.86 to −7.14 km s^-1 (dashed contour) which is within the same V_LSR range as that of the narrow-band data, and V_LSR from −7.14 to 22.93 km s^-1 (dotted contour) toward NML Cyg superposed on the 43 GHz continuum emission (solid contour) with peak position indicated by the star. The maser spots within the same V_LSR range as the narrow-band data are marked with circles, with size proportional to the logarithm of their flux densities. The V_LSR of the maser spots is color-coded as indicated by the color bar on the right side, which use the same range of V_LSR as other maser spots figures in this paper for comparison. All offsets are relative to the strongest maser emission at V_LSR of −4.66 km s^-1. The relative positions of the SiO maser and radio continuum emission is estimated to be accurate to ≈3 mas. Contour levels for integrated maser emission are 0.18 Jy beam^-1 × 2ⁿ,n = 0...5 and for the radio continuum are integer multiples of 0.10 mJy beam^-1. The restoring beam for the maser (dotted circle) and continuum (solid circle) emissions are indicated in the lower left corner. (This figure is available in color in electronic form.)