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Loading contentThe broad family of detectors that must be cooled to cryogenic temperatures — sometimes thousandths of a degree above absolute zero — so that thermal noise does not swamp the faint astronomical signal. Bolometers and MKIDs are cryogenic detectors; the technique is essential across the infrared, millimetre, and X-ray.
Facts on this topic will be cited from these primary and reference sources.
Ground-based optical/infrared observatory data and imagery.