K波段多目標攝譜儀(英語:K-band multi-object spectrograph,或 KMOS),是安裝在智利帕拉納天文台ESO的甚大望遠鏡「阿圖」(UT1,太陽)上的儀器。KMOS是一款多目標攝譜儀,能夠在紅外光下同時觀察24個物體,並繪製出它們的特性如何因地而異。它將提供關鍵數據,幫助瞭解星系在早期宇宙中是如何生長和演化的。
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