Share Email Print
cover

Proceedings Paper

Diamond machining of ZnSe grisms for the Near Infrared Imager and Slitless Spectrograph (NIRISS) onboard JWST
Author(s): Paul J. Kuzmenko; Steve L. Little; Loïc Albert; David A. Aldridge; René Doyon; Michael Maszkiewicz; Driss Touahri
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

LLNL diamond machined a ZnSe grism for spectroscopy of transiting exoplanets on NIRISS, a Canadian instrument that will fly on the James Webb Space Telescope. The grism operates over the wavelength range of 0.6 to 2.5 μm. It is cross-dispersed by a ZnS prism and has a resolving power in first order of ~700. The surface error over the full 29 x 30 mm grating aperture is 0.03 wave rms at 633nm. We measured a diffraction efficiency at 633 nm of 56% (nearly 88% after accounting for Fresnel reflection). The diffraction pattern is clean with no discernible ghosts.

Paper Details

Date Published: 7 August 2014
PDF: 14 pages
Proc. SPIE 9151, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation, 915159 (7 August 2014); doi: 10.1117/12.2054420
Show Author Affiliations
Paul J. Kuzmenko, Lawrence Livermore National Lab. (United States)
Steve L. Little, Lawrence Livermore National Lab. (United States)
Loïc Albert, Univ. de Montréal (Canada)
David A. Aldridge, COM DEV Canada (Canada)
René Doyon, Univ. de Montréal (Canada)
Michael Maszkiewicz, Canadian Space Agency (Canada)
Driss Touahri, COM DEV Canada (Canada)


Published in SPIE Proceedings Vol. 9151:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation
Ramón Navarro; Colin R. Cunningham; Allison A. Barto, Editor(s)

© SPIE. Terms of Use
Back to Top
PREMIUM CONTENT
Sign in to read the full article
Create a free SPIE account to get access to
premium articles and original research
Forgot your username?
close_icon_gray