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We collate active galactic nuclei (AGN) with reported detections of bothrelativistic reflection and ultra-fast outflows. By comparing the inclinationof the inner disc from reflection with the line-of-sight velocity of theoutflow, we show that it is possible to meaningfully constrain the geometry ofthe absorbing material. We find a clear relation between the velocity andinclination, and demonstrate that it can potentially be explained either bysimple wind geometries or by absorption from the disc surface. Due tosystematic errors and a shortage of high- quality simultaneous measurements ourconclusions are tentative, but this study represents a proof-of-concept thathas great potential.

Constraining the geometry of AGN outflows with reflection spectroscopy