Jadhav, YashashreeYashashreeJadhavRobinson, AndrewAndrewRobinsonAlmeyda, TrianaTrianaAlmeydaCURRAN, RACHEL LOUISERACHEL LOUISECURRANMARCONI, AlessandroAlessandroMARCONI2025-03-272025-03-2720210035-8711http://hdl.handle.net/20.500.12386/36957A galaxy merger is expected to cause the formation of a supermassive black hole (SMBH) binary, which itself eventually coalesces through the anisotropic emission of gravitational waves. This may result in the merged SMBH receiving a recoil kick velocity ~100-1000 kms<SUP>-1</SUP>, causing it to oscillate in the gravitational potential of the host galaxy. The luminous quasar E1821+643, identified as an SMBH recoil candidate via spectropolarimetry observations, shows Doppler shifting of the broad emission lines in direct and scattered light, consistent with a relative velocity of 2100 km s<SUP>-1</SUP> between the quasar nucleus and host galaxy. In this paper, we attempt to detect the expected spatial displacement using a combination of optical spectroastrometry and Hubble Space Telescope (HST) narrow-band images. The spectroastrometry reveals a relative spatial displacement between the quasar nucleus and the gas emitting the [O III] λλ4959, 5007 lines of ~130 mas (~580 pc) to the north-west. Our HST images resolve the [O III] emission on sub-arcsecond scales, showing that it is asymmetrically distributed, extending to radial distances ~0.5-0.6 arcsec from the nucleus in a wide arc running from the north-east around to the west. A simulated spectroastrometry observation based on the HST [O III] image indicates that only a small fraction of the measured displacement can be attributed to the asymmetric [O III] emission. This displacement therefore appears to be a real spatial offset of the quasar nucleus with respect to the narrow-line region, presumed to be located at the host galaxy centre, further supporting the interpretation that a post-merger gravitational recoil of the SMBH has occurred in E1821+643.STAMPAenArticle10.1093/mnras/stab21762-s2.0-85114994583https://academic.oup.com/mnras/article/507/1/484/6330460?login=falsehttp://arxiv.org/abs/2107.14711v12021MNRAS.507..484JFIS/05 - ASTRONOMIA E ASTROFISICA