Transition-edge sensor: Difference between revisions

Revision as of 09:34, 23 October 2019

Revision as of 03:33, 10 September 2020

Line 27:

==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]], the [[Spider (polarimeter)|Spider polarimeter]] and, the X-IFU instrument of the [[Advanced Telescope for High Energy Astrophysics]] satellite, and the future [https://link.springer.com/article/10.1007/s10909-019-02329-w LiteBIRD] Cosmic Microwave Background polarization experiment

==See also==