In the last decade, cryogenic bolometers have provided increasingly improved resolution
and sensitivity in particle and radiation detectors. Thermal particle detectors have proven …

Superconducting detector arrays have become the standard technology for the current
generation of millimeter-wave and submm-wave astronomical instruments on individual …

CMB-S4 is a proposed experiment to map the polarization of the Cosmic Microwave
Background (CMB) to nearly the cosmic variance limit for angular scales that are accessible …

Aims. Future astrophysics and cosmic microwave background space missions operating in
the far-infrared to millimetre part of the spectrum will require very large arrays of ultra …

Aims. Future actively cooled space-borne observatories for the far-infrared, loosely defined
as a 1–10 THz band, can potentially reach a sensitivity limited only by background radiation …

Microwave kinetic inductance detectors (MKIDs) are thin-film, cryogenic, superconducting
resonators. Incident Cooper pair-breaking radiation increases their kinetic inductance …

The Prime-Cam instrument on the Fred Young Submillimeter Telescope (FYST) is expected
to be the largest deployment of millimeter and submillimeter sensitive kinetic inductance …

Terahertz spectrometers with a wide instantaneous frequency coverage for passive remote
sensing are enormously attractive for many terahertz applications, such as astronomy …

In millimeter and submillimeter-wave radiometric imaging systems, a persistent goal is the
increase in the speed of acquisition of the image while maintaining a high sensitivity …

Next generation sub-mm imaging instruments require kilo-pixel focal plane arrays filled with
background limited detectors. Microwave kinetic inductance detectors (MKIDs) are a state-of …