Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond
arXiv:1803.03280 · doi:10.1007/s10909-018-1949-5
Abstract
Microwave Kinetic Inductance Detectors (MKIDs) provide a compelling path forward to the large-format polarimeter, imaging, and spectrometer arrays needed for next-generation experiments in millimeter-wave cosmology and astronomy. We describe the development of feedhorn-coupled MKID detectors for the TolTEC millimeter-wave imaging polarimeter being constructed for the 50-meter Large Millimeter Telescope (LMT). Observations with TolTEC are planned to begin in early 2019. TolTEC will comprise 7,000 polarization sensitive MKIDs and will represent the first MKID arrays fabricated and deployed on monolithic 150 mm diameter silicon wafers -- a critical step towards future large-scale experiments with over detectors. TolTEC will operate in observational bands at 1.1, 1.4, and 2.0 mm and will use dichroic filters to define a physically independent focal plane for each passband, thus allowing the polarimeters to use simple, direct-absorption inductive structures that are impedance matched to incident radiation. This work is part of a larger program at NIST-Boulder to develop MKID-based detector technologies for use over a wide range of photon energies spanning millimeter-waves to X-rays. We present the detailed pixel layout and describe the methods, tools, and flexible design parameters that allow this solution to be optimized for use anywhere in the millimeter and sub-millimeter bands. We also present measurements of prototype devices operating in the 1.1 mm band and compare the observed optical performance to that predicted from models and simulations.
arXiv comment7 pages, 4 figures, 1 table. Submitted to Journal of Low Temperature Physics
References in corpus (10)
- Low Loss Superconducting Titanium Nitride Coplanar Waveguide Resonators
- ARCONS: A 2024 Pixel Optical through Near-IR Cryogenic Imaging Spectrophotometer
- The NIKA2 instrument, a dual-band kilopixel KID array for millimetric astronomy
- Photon noise limited radiation detection with lens-antenna coupled Microwave Kinetic Inductance Detectors
- Proximity-Coupled Ti/TiN Multilayers for use in Kinetic Inductance Detectors
- Photon-noise limited sensitivity in titanium nitride kinetic inductance detectors
- NIKEL_AMC: Readout electronics for the NIKA2 experiment
- The Next Generation BLAST Experiment
- Status of MUSIC, the MUltiwavelength Sub/millimeter Inductance Camera
- Optical Demonstration of THz, Dual-Polarization Sensitive Microwave Kinetic Inductance Detectors
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