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Contrast Measurements of the Microshutter Arrays for the NIRspecWe have been developing programmable microshutter arrays for the Near Infrared Spectrometer (NIRSpec) on the James Webb Space telescope (JWST). These arrays are an enabling technology that allows to turn NIRSpec into a powerful multi-object spectrometer and tremendously increase its efficiency. The arrays are essentially 2D programmable masks that are designed to operate at cryogenic temperatures of JWST. The primary optical characteristic of the microshutter array is a contrast, that is defined as a ratio of the transmitted light intensity through open shutters to the intensity of the transmitted light through the closed shutters. To eliminate the noise and confusion from other sources in the field of view and therefore to improve the detection limit, the contrast provided by the microshutter array should be very high, with the goal of 10,000. The test system that we have developed specifically for the purpose of the high contrast characterization of the microshutter array devices has been used to test several microshutter arrays. It is capable of measuring contrast values of up to 10^5 and therefore can reliably measure contrast values of the arrays that satisfy the requirements. The arrays have been characterized for the contrast ratio and its behavior with temperature and other array operating parameters. The arrays that we have tested meet or exceed the NiRSpec requirements.
Document ID
20080031150
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Kutyrev, Alexander
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Chambers, J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Moseley, S. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Rapchun, D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 24, 2013
Publication Date
January 7, 2008
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: American Astronomical Society
Location: Austin, TX
Country: United States
Start Date: January 7, 2008
End Date: January 10, 2008
Sponsors: American Astronomical Society
Funding Number(s)
CONTRACT_GRANT: NNG06EO90A
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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