Translator Disclaimer
24 August 2018 Progress towards ultra sensitive KIDs for future far-infrared missions: a focus on recombination times
Author Affiliations +
Future generations of far-infrared (FIR) telescopes will need detectors with noise-equivalent powers on the order of 5x10-20 W/Hz1/2 in order to be photon background limited by astrophysical sources. One such mission concept in development is the Galaxy Evolution Probe (GEP), which will characterize galaxy formation and evolution from z=0 to beyond z=4. Kinetic inductance detectors (KIDs) have been baselined for the GEP for spectroscopy and imaging science between 10 μm and 400 μm due to their intrinsic frequency multiplexability and simple readout schemes. We focus on quasiparticle recombination times as a strategy for increasing detector responsivities to move towards the NEP requirements of the GEP. We present a new model for quantifying time constants from the responses of detectors to pulses of light, and test this model on a 40 nm thick ¼ λ Al coplanar waveguide KID. We intend to use this measurement scheme to quantify the dependence of the quasiparticle recombination time on Al thickness.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Adalyn Fyhrie, Jonas Zmuidzinas, Jason Glenn, Peter Day, Henry G. LeDuc, and Christopher McKenney "Progress towards ultra sensitive KIDs for future far-infrared missions: a focus on recombination times", Proc. SPIE 10708, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy IX, 107083A (24 August 2018);


Development of DESHIMA a redshift machine based on a...
Proceedings of SPIE (September 27 2012)
MKID multicolor array status and results from DemoCam
Proceedings of SPIE (July 15 2010)
MKID development for SuperSpec an on chip, mm wave,...
Proceedings of SPIE (September 27 2012)
Superconducting kinetic inductance photon detectors
Proceedings of SPIE (December 18 2002)

Back to Top