Poster + Paper
21 August 2024 Characterizing fabrication quality and UV performance of UV gratings
Author Affiliations +
Conference Poster
Abstract
Ultraviolet (UV, 900−2000 Å) spectroscopy plays a vital role in studying exoplanets. Future UV spectrographs will require large-format, high-performance gratings (R > 104). Unfortunately, measuring the UV performance of a large-format grating from 900−2000˚ Å is resource-intensive and requires large special vacuum facilities, hampering UV grating development. An efficient characterization process will save time and reduce costs, facilitating the development of blazed UV gratings for next-gen UV space telescopes. This work is part of an effort to determine if we can leverage trends found between measured UV grating performance (on small stamp-size gratings) and the grating’s intrinsic, fabricated characteristics to estimate the expected performance of large-format UV gratings. Here, we present a pilot study using an 855nm period grating. We characterize the grating’s fabrication quality via interferometry and single-point metrology. Finally, we describe measurements of the grating’s diffraction efficiency that will be conducted later this year.
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jared A. B. Termini, Keri Hoadley, Casey DeRoo, Cecilia Fasano, Paul Scowen, Manuel Quijada, Mateo Batkis, Javier Del Hoyo, Luis Rodriguez-de-Marcos, Erika Hamden, and Jessica Li "Characterizing fabrication quality and UV performance of UV gratings", Proc. SPIE 13093, Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray, 1309342 (21 August 2024); https://doi.org/10.1117/12.3016276
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KEYWORDS
Ultraviolet radiation

Blazed gratings

Surface roughness

Fabrication

Diffraction gratings

Coating

Optical gratings

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