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The Kunlun Infrared Sky Survey will be the first comprehensive exploration ofthe time varying Universe in the infrared. A key feature in optimizing thescientific yield of this ambitious research program is the choice of the surveypassband. In particular the survey aims to maximally exploit the unique thermaland atmospheric conditions pertaining to the high Antarctic site. By simulatingthe expected signal-to-noise for varying filter properties within the so-called"K_DARK" 2.4um window, filter performance can be tuned and best-case designsare given covering a range of conditions.

Optimising the K dark filter for the Kunlun Infrared Sky Survey