Far-infrared spectroscopy probes the cold and dust-enshrouded regions of the Universe by measuring electromagnetic radiation in the 30–300 μm band. This regime encompasses the principal cooling lines ...
Infrared astronomy relies on specialised instruments designed to detect and analyse radiation from approximately 1 µm to several hundred microns in wavelength. Key components include cooled detector ...
IIIF provides researchers rich metadata and media viewing options for comparison of works across cultural heritage collections. Visit the IIIF page to learn more. This spectroscope was designed to be ...
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