Transition-edge sensor: Difference between revisions

Revision as of 13:23, 30 October 2017

Revision as of 09:19, 22 February 2019

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==Applications==

TES arrays are becoming increasingly common in physics and astronomy experiments such as [[James Clerk Maxwell Telescope#SCUBA-2|SCUBA-2]], the HAWC+ instrument on the [[Stratospheric Observatory for Infrared Astronomy]], the [[Atacama Cosmology Telescope]], the [[Cryogenic Dark Matter Search]], the [[Cryogenic Rare Event Search with Superconducting Thermometers]], [[the E and B Experiment]], the [[South Pole Telescope]], and the [[Spider (polarimeter)|Spider polarimeter]] and the X-IFU instrument of the [[Advanced Telescope for High Energy Astrophysics]] satellite.

==See also==