학술논문
Detector Systems Engineering for Extremely Large Instruments
Document Type
Working Paper
Author
George, Elizabeth M.; Bezawada, Naidu; Ives, Derek; Mehrgan, Leander; Accardo, Matteo; Alvarez, Domingo; Brinkmann, Martin; Conzelmann, Ralf; Cumani, Claudio; Downing, Mark; Engelhardt, Max; Haug, Marcus; Hopgood, Joshua; Geimer, Christoph; Iwert, Olaf; Klein, Barbara; Mandla, Christopher; Müller, Eric; Ramsay, Suzanne; Reyes, Javier; Richerzhagen, Mathias; Serra, Benoît; Seidel, Matthias; Stegmeier, Jörg; Todorovic, Mirko
Source
Proc. SPIE 11454, X-Ray, Optical, and Infrared Detectors for Astronomy IX, 114541Y (13 December 2020)
Subject
Language
Abstract
The scientific detector systems for the ESO ELT first-light instruments, HARMONI, MICADO, and METIS, together will require 27 science detectors: seventeen 2.5 $\mu$m cutoff H4RG-15 detectors, four 4K x 4K 231-84 CCDs, five 5.3 $\mu$m cutoff H2RG detectors, and one 13.5 $\mu$m cutoff GEOSNAP detector. This challenging program of scientific detector system development covers everything from designing and producing state-of-the-art detector control and readout electronics, to developing new detector characterization techniques in the lab, to performance modeling and final system verification. We report briefly on the current design of these detector systems and developments underway to meet the challenging scientific performance goals of the ELT instruments.
Comment: Proceedings of the SPIE Astronomical Telescopes and Instrumentation Conference 2020
Comment: Proceedings of the SPIE Astronomical Telescopes and Instrumentation Conference 2020