Cryogenic particle detection

By C. Enss. 2005

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A White Paper on keV sterile neutrino Dark Matter (2016, background): “Presently the detectors that can detect with the highest precision energy input below 3 keV, as is needed for the calorimetric measurement of the 163Ho, are low temperature microcalorimeters [938].”
The physics of superconducting microwave resonators (2008, background): “Currently the Cryogenic Dark Matter Search (CDMS) experiment uses 19 Ge targets (a total mass of 4.75 kg) and 11 Si targets (a total mass of 1.1 kg), with TES phonon sensors covering the surface of each target.”
THE ATACAMA COSMOLOGY TELESCOPE: THE POLARIZATION-SENSITIVE ACTPol INSTRUMENT (2016, methodology): “Changes in radiation power are detected using superconducting TES bolometers (Lee et al. 1996; Irwin & Hilton 2005).”
Lumped Element Kinetic Inductance Detectors (2008, background): “TES bolometers are limited in sensitivity by the thermal isolation of the absorber and limited in the speed of response by the heat capacity of the absorber [1].”
SCUBA-2: the 10 000 pixel bolometer camera on the James Clerk Maxwell Telescope (2013, methodology): “The SCUBA-2 sub-arrays are based on transition edge sensors and time-division SQUID-based multiplexers developed at the National Institute of Standards and Technology in Boulder, Colorado (Irwin & Hilton 2005).”