Transition-edge sensor: Difference between revisions

Revision as of 20:31, 18 March 2014

Revision as of 12:23, 11 June 2014

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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 [[Atacama Cosmology Telescope]], the [[Cryogenic Dark Matter Search]], [[the E and B Experiment]], the [[South Pole Telescope]], and the [[Spider (polarimeter)|Spider polarimeter]].

==References==

{{reflist}}

==See also==

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*[[Bolometer]]

*[[Cryogenic particle detectors]]

==References==

{{reflist}}

[[Category:Superconducting detectors]]