Paper
9 August 2016 Wide-Field InfraRed Survey Telescope (WFIRST) slitless spectrometer: design, prototype, and results
Author Affiliations +
Abstract
The slitless spectrometer plays an important role in the WFIRST mission for the survey of emission-line galaxies. This will be an unprecedented very wide field, HST quality 3D survey of emission line galaxies1. The concept of the compound grism as a slitless spectrometer has been presented previously. The presentation briefly discusses the challenges and solutions of the optical design, and recent specification updates, as well as a brief comparison between the prototype and the latest design. However, the emphasis of this paper is the progress of the grism prototype: the fabrication and test of the complicated diffractive optical elements and powered prism, as well as grism assembly alignment and testing. Especially how to use different tools and methods, such as IR phase shift and wavelength shift interferometry, to complete the element and assembly tests. The paper also presents very encouraging results from recent element tests to assembly tests. Finally we briefly touch the path forward plan to test the spectral characteristic, such as spectral resolution and response.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Qian Gong, David A. Content, Margaret Dominguez, Thomas Emmett, Ulf Griesmann, John Hagopian, Jeffrey Kruk, Catherine Marx, Bert Pasquale, Thomas Wallace, and Arthur Whipple "Wide-Field InfraRed Survey Telescope (WFIRST) slitless spectrometer: design, prototype, and results", Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 990412 (9 August 2016); https://doi.org/10.1117/12.2231665
Lens.org Logo
CITATIONS
Cited by 10 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Interferometers

Chemical elements

Computer generated holography

Diffraction

Wavefronts

Prototyping

Optical design

Back to Top