Microwave kinetic inductance detectors (MKIDs) provide a compelling path forward to the
large-format polarimeter, imaging, and spectrometer arrays needed for next-generation …

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 …

CCAT-prime will be a 6-meter aperture telescope operating from sub-mm to mm
wavelengths, located at 5600 meters elevation on Cerro Chajnantor in the Atacama Desert …

We present a wafer trimming technique for producing superconducting micro-resonator
arrays with highly uniform frequency spacing. With the light-emitting diode mapper …

The Cerro Chajnantor Atacama Telescope-prime (CCAT-prime) is a new 6-m, off-axis, low-
emissivity, large field-of-view submillimeter telescope scheduled for first light in the last …

Microwave kinetic inductance detectors, or MKIDs (Day, Leduc, Mazin, et al. 2003;
Zmuidzinas, 2012), are superconducting resonators suitable for a wide variety of photon and …

We demonstrate microwave kinetic inductance detectors (MKIDs) whose sensitivity is limited
by photon noise at signal frequencies as low as 50 mHz. The subhertz part of the detection …

The Next Generation Balloon-borne Large Aperture Submillimeter Telescope (BLAST-TNG)
is a submillimeter mapping experiment planned for a 28 day long-duration balloon (LDB) …

The Fred Young Submillimeter Telescope (FYST) at the Cerro-Chajnantor Atacama
Telescope prime (CCATprime) Facility will host Prime-Cam as a powerful, first generation …

Aims. Lumped-element kinetic inductance detectors (LEKIDs) are an attractive technology
for millimeter-wave observations that require large arrays of extremely low-noise detectors …