Abstract
The XENON family of experiments have been at the forefront of direct dark matter searches for weak-scale dark matter for more than fifteen years. In this time, the program has scaled from a few-kilogram pathfinder detector to the current XENONnT holding 8.6 tonne of liquid xenon. Innovations in xenon handling, material selection and purification have allowed each detector generation to feature a lower background rate than the previous.
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