Array Characterization
To characterize the performance of the LW13 and LW15 arrays, the first step is to calibrate the data. Calibration involves the calculation of the multiplexer gain, diode capacitance to determine the ADU to electron conversion, and non-linearity measuremen
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Mario Cabrera
Development of 15 Micron Cutoff Wavelength HgCdTe Detector Arrays for Astronomy
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Mario Cabrera
Development of 15 Micron Cutoff Wavelength HgCdTe Detector Arrays for Astronomy Doctoral Thesis accepted by the University of Rochester, USA
Mario Cabrera Glenn Dale MD, USA
ISSN 2190-5053 ISSN 2190-5061 (electronic) Springer Theses ISBN 978-3-030-54240-5 ISBN 978-3-030-54241-2 (eBook) https://doi.org/10.1007/978-3-030-54241-2 © Springer Nature Switzerland AG 2020 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such name
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