  KELT-9b is an ultra-hot Jupiter observed to be undergoing extreme mass loss.
Its A0-type host star has a radiative envelope, which makes its surface layers
prone to retaining recently accreted material. To search for potential signs of
planetary material polluting the stellar surface, we carry out the most
comprehensive chemical characterisation of KELT-9 to-date. New element
detections include Na and Y, which had previously been detected in the
ultra-hot Jupiter but not studied in the star; these detections complete the
set of nine elements measured in both star and planet. In comparing KELT-9 with
similar open cluster stars we find no strong anomalies. This finding is
consistent with calculations of photospheric pollution accounting for stellar
mixing and using observationally estimated KELT-9b mass loss rates. We also
rule out recent, short-lived intensive mass transfer such as the stellar
ingestion of an Earth-mass exomoon.
