Detectors for the James Webb Space Telescope Near-Infrared Spectrograph I: Readout Mode, Noise Model, and Calibration Considerations Bernard J. Rauscher and Ori Fox1 NASA Goddard Space Flight Center, Greenbelt, MD 20771
[email protected] Pierre Ferruit2,3 Universit´ede Lyon, Lyon, F-69003, France Robert J. Hill8, Augustyn Waczynski4, Yiting Wen6, Wei Xia-Serafino4, Brent Mott, David Alexander, Clifford K. Brambora, Rebecca Derro, Chuck Engler, Matthew B. Garrison, Thomas Johnson, Sridhar S. Manthripragada, James M. Marsh, Cheryl Marshall, Robert J. Martineau, Kamdin B. Shakoorzadeh7, Donna Wilson, Wayne D. Roher5, and Miles Smith NASA Goddard Space Flight Center, Greenbelt, MD 20771 Craig Cabelli, James Garnett, Markus Loose, Selmer Wong-Anglin, Majid Zandian, and Edward Cheng8 Teledyne Imaging Sensors, 5212 Verdugo Way, Camarillo, CA 93012 arXiv:0706.2344v1 [astro-ph] 15 Jun 2007 Timothy Ellis, Bryan Howe, Miriam Jurado, Ginn Lee, John Nieznanski, Peter Wallis, and James York ITT Space Systems Division, 1447 St. Paul Street, Rochester, NY, 14653 Michael W. Regan Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 Donald N.B. Hall and Klaus W. Hodapp –2– Institute for Astronomy, 640 North A´ohoku Place, #209, Hilo HI 96720 and Torsten B¨oker, Guido De Marchi, Peter Jakobsen, and Paolo Strada ESTEC, Astrophysics Division, Postbus 299, Noordwijk, NL2200 AG, Netherlands Received ; accepted Accepted by Publications of the Astronomical Society of the Pacific 1Also at Department of Astronomy, University of Virginia,