  We consider the boosted dark matter solution of the XENON1T excess to
constrain the framework through loop-generated processes. The interaction of
the boosted dark matter component, which sources the signal, effectively
couples the cold dark matter background to the electrons, making it potentially
visible in the electron recoil searches. Similarly, once the radiative
corrections due to the Standard Model are taken into account, dark matter also
scatters on quarks and becomes observable in nuclear recoil measurements. By
analysing these processes, we find that the current direct detection
constraints exclude the upper mass range selected by the anomaly if the boosted
component is generated through dark matter annihilation.
