“…The emission was found in the context of a series of experiments on the emission and absorption features of liquid noble gases [1,3,4,5]. This study was motivated by the fact that liquid rare gases are presently often used in large quantities as the detector material in rare event physics, e.g., the search for the neutrinoless double-beta decay (GERDA Phase II uses a liquid argon veto [6], EXO uses liquid xenon [7]) and the direct dark matter search (Liquid argon: WArP [8], ArDM [9,10], DarkSide [11]; Liq-arXiv:1511.07722v1 [physics.ins-det] 24 Nov 2015 uid xenon: XENON100 [12], LUX [13]).…”