Lumped element kinetic inductance detectors for space applications

Abstract : Kinetic Inductance Detectors (KIDs) are now routinely used on ground-based telescopes. These large arrays, deployed in formats up to several kilopixels, exhibit state-of-the-art performance at millimeter (e.g. 120-300 GHz, NIKA and NIKA2) and sub-millimeter (e.g. 350-850 GHz, AMKID) wavelengths. We have studied in detail the interaction of ionizing particles (muons, alphas, x-rays) with KID arrays of hundreds of pixels designed for Cosmic Microwave Background observations. We have also set up a dedicated cryostat in which we reproduce typical observing conditions of a space-borne CMB observation. We will report the details and conclusions from a large number of measurements.
Type de document :
Communication dans un congrès
SPIE Conference Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, Jun 2016, Edinburgh, United Kingdom. Proc. SPIE Millimeter, Submillimeter, and Far-Infrared Detectoers and Instrumentation for Astronomy VIII, 9914, pp.99140N, 2016, 〈10.1117/12.2231758〉
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http://hal.in2p3.fr/in2p3-01339829
Contributeur : Emmanuelle Vernay <>
Soumis le : jeudi 30 juin 2016 - 09:36:08
Dernière modification le : jeudi 11 janvier 2018 - 06:26:41

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A. Monfardini, J. Baselmans, A. Benoit, A. Bideaud, O. Bourrion, et al.. Lumped element kinetic inductance detectors for space applications. SPIE Conference Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, Jun 2016, Edinburgh, United Kingdom. Proc. SPIE Millimeter, Submillimeter, and Far-Infrared Detectoers and Instrumentation for Astronomy VIII, 9914, pp.99140N, 2016, 〈10.1117/12.2231758〉. 〈in2p3-01339829〉

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