Multiple space missions currently under study require high-performing detectors at mid-infrared wavelengths from 2 to 20 µm. However, the future availability of the IBC detectors used for JWST is in doubt, and HgCdTe detectors have difficulties at longer wavelengths. Superconducting detectors are therefore being considered as a solution to fill this technology gap. Superconducting nanowire single-photon detectors (SNSPDs) are particularly advantageous, because they are true photon-counting detectors with digital-like output signals and low dark count rates. These features make them very stable for applications like exoplanet transit spectroscopy and able to operate in photon-starved environments for applications like nulling interferometry. We have recently demonstrated SNSPDs with high internal detection efficiency at wavelengths as long as 29 µm. This talk will provide an overview of the current state of mid-IR SNSPDs and lay out the future steps needed to adapt them for exoplanet science missions.
Superconducting nanowire single-photon detectors (SNSPDs) have become the highest-performing type of single-photon detector, with demonstrations of near-unity detection efficiency, GHz count rate, and a broad wavelength range from UV to mid-IR. Scaling these detectors to large areas and pixel counts with minimal tradeoffs in their detection properties would expand the use case of SNSPDs to applications like astronomical spectroscopy, quantum imaging, or dark matter searches. In this talk, I will discuss a thermal coupling scheme enabling these large detector arrays and several array architectures to target the requirements of specific applications.
Superconducting nanowire single-photon detectors (SNSPDs) have become the gold standard for single photon detection at telecom wavelengths, and their high efficiency, high dynamic range, low timing jitter, and low dark count rates make them ideal for quantum applications. Many use cases benefit from arrays of SNSPDs, whether it’s to enable number resolution, to access higher maximum count rates, to cover larger active areas, or to provide imaging or spectroscopy capabilities. SNSPD array design typically involves a tradeoff between number of channels, active area, and timing properties. In this talk, I will discuss several applications of SNSPD arrays and describe how the applications’ different requirements affect the array and system-level design choices.
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