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, talking and hearing. No special vision requirements. Must be able to lift or exert force up to (10) pounds. WORK ENVIRONMENT: Laboratory environment. Moderate Noise Special Conditions Posting Details
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Demands: No physical demands Work Environment: No significant exposure or noise levels. Office/Laboratory/Clinical Environment Special Conditions Posting Details Posting Number 25ST0742 Posting Open Date
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, at QCD Labs, we have recently developed the most coherent transmon qubits , the lowest-noise bolometers and highest-resolution calorimeters, and shown that they can be used to read out the state of a
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, sitting, walking, talking, and hearing. Experience working in a fast-paced environment. Lab environment. Lifting to 25lbs. Work Environment: Open office environment. Moderate noise and foot traffic
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: Standing, sitting, walking, talking and hearing. No special vision requirements. Lifting up to 25 lbs. WORK ENVIRONMENT: Lab environment with moderate noise. Exposure to blood, excrement, antineoplastic
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DEMANDS: Standing, sitting, walking, talking and hearing. No special vision requirements. Lifting up to 25 lbs. WORK ENVIRONMENT: Lab environment with moderate noise. Exposure to blood, excrement
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, and use of instrumentation including microscopes. WORK ENVIRONMENT; Laboratory environment. Low to moderate noise. Universal safety precautions are mandatory. Special Conditions Posting Details Posting
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), latch-ups, and the total ionising dose on spiking neural network performance. develop and test fault mitigation strategies, such as spike-based redundancy, reconfigurable neural routing, noise-aware
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University of North Carolina at Chapel Hill | Chapel Hill, North Carolina | United States | 3 months ago
coaddition for faint sources and structure. Argus is a massively multiplexed array of 900 small-aperture telescopes, able to cover a combined 8,000 square degrees of sky with 55 gigapixels of low-noise CMOS
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University of North Carolina at Chapel Hill | Chapel Hill, North Carolina | United States | 3 months ago
beyond. Argus is a massively multiplexed array of 900 small-aperture telescopes, able to cover a combined 8,000 square degrees of sky with 55 gigapixels of low-noise CMOS detectors. This enormous field