An optical device that cuts a two-dimensional astronomical image into multiple narrow strips and rearranges them into a linear format suitable for spectroscopy. This allows efficient use of spectrograph entrance slits while preserving spatial information from extended objects like galaxies or nebulae.
Descriptive compound of 'image' from Latin 'imago' (likeness) and 'slicer' from Old French 'esclicier' (to split). The term emerged in the 1980s as astronomers developed sophisticated optical systems to maximize the efficiency of expensive spectrographic observations by reformatting telescope images into optimal shapes for spectral analysis.
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