Titlebook: Improving the Resolving Power of Ultraviolet to Near-Infrared Microwave Kinetic Inductance Detectors; Nicholas Zobrist Book 2022 The Edito

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Data Analysis,ctivity 27:1–4, 2017). Understanding how the filtering method breaks down for ultraviolet to near-infrared MKIDs allows us to modify the traditionally used analysis method for these detectors at the end of the chapter.

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Conclusions,nderstanding of exoplanets. In addition to simplifying the required optics needed to support multiple non-energy resolving detectors, photon counting opens the door for powerful new methods which allow us to detect exoplanets in increasingly difficult conditions [., .].

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Detector and Readout Noise,photons are being absorbed by the detector. We use this property to simplify the noise analysis since we can study it without the detector being illuminated. While not all noise sources are additive, luckily, most of the ones that affect MKIDs fall into this category.

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Introduction and Motivation,different fields. In bio-analysis research, there is demand for detectors that can measure fast, low-light biological processes with energy sensitivity (Niwa et al., Sci Rep 7:45660, 2017). Axion and hidden photon dark matter searches, too, could benefit from these kinds of detectors by expanding th

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Detector and Readout Noise,sources. In this chapter, we discuss additive noise which can be understood as a realization of a random variable with zero mean added to our expected signal. This type of noise is not necessarily stationary since its magnitude can change during the photon response, but it does exist whether or not