Composite image of HD 163296 shows two jets detected by MUSE, superimposed to the disk detected by ALMA at 1.2 mm (Andrews et al. 2018; Isella et al. 2018). The NE jet and SW jet are traced by [SII] 673 nm and Hα lines, respectively, and are smoothed with a Gaussian kernel of 2 pixels in radius. The arc-like structure near the SW jet is the blob ghost caused by the instrument (see Appendix A). The inset box of Hα image shows the inner most region. The magenta cross marks the stellar position.