Detectors for theJames Webb Space TelescopeNear‐Infrared Spectrograph. I. Readout Mode, Noise Model, and Calibration Considerations

Author:

Rauscher Bernard J.,Fox Ori,Ferruit Pierre,Hill Robert J.,Waczynski Augustyn,Wen Yiting,Xia‐Serafino Wei,Mott Brent,Alexander David,Brambora Clifford K.,Derro Rebecca,Engler Chuck,Garrison Matthew B.,Johnson Thomas,Manthripragada Sridhar S.,Marsh James M.,Marshall Cheryl,Martineau Robert J.,Shakoorzadeh Kamdin B.,Wilson Donna,Roher Wayne D.,Smith Miles,Cabelli Craig,Garnett James,Loose Markus,Wong‐Anglin Selmer,Zandian Majid,Cheng Edward,Ellis Timothy,Howe Bryan,Jurado Miriam,Lee Ginn,Nieznanski John,Wallis Peter,York James,Regan Michael W.,Hall Donald N. B.,Hodapp Klaus W.,Böker Torsten,De Marchi Guido,Jakobsen Peter,Strada Paolo

Publisher

IOP Publishing

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference19 articles.

1. Arendt, R. G., Fixsen, D. J. & Moseley, S. H. 2002, in ASP Conf. Ser. 281, Astronomical Data Analysis Software and Systems XI, ed. D. A. Bohlender, D. Durand, & T. H. Handley (San Francisco: ASP), 217

2. Bevington, P. R. 1969, Data Reduction and Analysis for the Physical Sciences (New York: McGraw Hill)

3. Further characterization of Rockwell Scientific LWIR HgCdTe detector arrays

4. Brice, J. C. 1987, Properties of Mercury Cadmium Telluride, ed. J. Brice & P. Capper (London: IEE)

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