Presentation
16 December 2020 Fabry-Perot interferometer for high spectral resolution in the infrared and submillimeter
Author Affiliations +
Abstract
HIRMES, SOFIA’s third generation science instrument, delivers spectroscopy at wavelengths between 25 and 122 um and resolving powers (RP) between 600 and 100,000. The detectors arrays are background-limited transition edge sensed bolometers. Here we focus on the development, testing, and performance of the series of 8 tunable cryogenic scanning Fabry-Perot interferometers (FPI) that deliver the imaging (RP = 2000), and the long-slit medium resolution (RP = 10,000) and high resolution (RP = 100,000) spectroscopic modes. The FPIs use free-standing metal meshes mirrors, flexible parallelogram translations stages, PZTs and/or cryomoters for displacement. and capacitive sensors for displacement measure.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Thomas Nikola, Gordon J. Stacey, Matthew Greenhouse, Alexander Kutyrev, James G. Douthit, Charles Henderson, George E. Gull, Wen-Ting Hsieh, Ellen Lee, and Kayla M Rossi "Fabry-Perot interferometer for high spectral resolution in the infrared and submillimeter", Proc. SPIE 11453, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X, 114530E (16 December 2020); https://doi.org/10.1117/12.2561869
Advertisement
Advertisement
KEYWORDS
Fabry–Perot interferometry

Cryogenics

Image resolution

Mirrors

Spatial resolution

Infrared astronomy

Infrared spectroscopy

RELATED CONTENT

Origins Space Telescope integration and testing
Proceedings of SPIE (December 13 2020)
Stratospheric Observatory for Infrared Astronomy (SOFIA)
Proceedings of SPIE (September 14 2016)
ASTRO-F mission
Proceedings of SPIE (March 05 2003)

Back to Top