We present a systematic study of the change in work function of noble metal ͑111͒ surfaces ͑Cu, Ag, Au͒ when being covered with a monolayer of a rare gas ͑Ar, Kr, Xe͒. Using a Kelvin probe the experiments show a decrease of the work function of the adsorbate covered system compared to the clean metal surface, in agreement with physisorption theory. The difference in work function depends both on the substrate and adsorbate being the highest for the Xe/ Cu system and the lowest for Ar/ Au. A comparison is performed with angle-resolved ultraviolet photoemission spectroscopy data using the binding energy shift of the ͑111͒ surface states of the same adsorbate/substrate systems, and with density functional calculations on simple model systems.