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JWST near infrared detectors: latest test results
Author(s) -
Erin C. Smith,
Bernard J. Rauscher,
David Alexander,
Brian L. Clemons,
Chuck Engler,
Matthew Garrison,
Robert Hill,
Thomas E. Johnson,
Don J. Lindler,
Sridhar Manthripragada,
Cheryl J. Marshall,
Brent Mott,
Thomas M. Parr,
Wayne D. Roher,
Kamdin B. Shakoorzadeh,
R. Schnurr,
Augustyn Waczynski,
Yiting Wen,
Donna V. Wilson,
Markus Loose,
Giorgio Bagnasco,
Torsten Böker,
Guido De Marchi,
Pierre Ferruit,
P. Jakobsen,
Paolo Strada
Publication year - 2009
Publication title -
proceedings of spie, the international society for optical engineering/proceedings of spie
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.192
H-Index - 176
eISSN - 1996-756X
pISSN - 0277-786X
DOI - 10.1117/12.826399
Subject(s) - detector , infrared , remote sensing , computer science , optics , physics , geology , telecommunications
The James Webb Space Telescope, an infrared-optimized space telescope being developed by NASA for launch in 2014, will utilize cutting-edge detector technology in its investigation of fundamental questions in astrophysics. JWST's near infrared spectrograph, NIRSpec utilizes two 2048 × 2048 HdCdTe arrays with Sidecar ASIC readout electronics developed by Teledyne to provide spectral coverage from 0.6 microns to 5 microns. We present recent test and calibration results for the "pathfinder NIRSpec detector subsystem" as well as data processing routines for noise reduction and cosmic ray rejection.

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