H-AMR simulation of accretion disk tilted by 30 degrees w.r.t. the black hole spin direction, ray-traced by using BHOSS. We look with an observer inclination angle of 90 degrees, or "edge-on" with respect to the outer disk at an observer frequency of 230 GHz. The thin line in front of the photon ring is the signature of a jet launched from the black hole-disk system. The image at 230 GHz is vividly different from a non-tilted accretion disk.

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