Poster + Paper
31 August 2022 Determining the efficiency of a cryogenic far-infrared diffraction grating spectrometer used as a post-dispersing module for a high-resolution spectrometer
Alicia M. Anderson, David A. Naylor, Brad G. Gom, Ian T. Veenendaal, Adam J. Christiansen, Willem Jellema, Peter A. R. Ade
Author Affiliations +
Conference Poster
Abstract
Recent advances in far-infrared detector technology have led to increases in raw sensitivity of more than an order of magnitude over previous state-of-the-art detectors. With such sensitivity, photon noise becomes the dominant noise component, even when using cryogenically cooled optics, unless a method of restricting the spectral bandpass is employed. The leading instrument concept features reflecting grating spectrometers to post-disperse the light that has been modulated by a polarizing Fourier transform spectrometer (FTS) onto a detector array, thereby reducing the photon noise on each detector. This paper describes the development of a cryogenic (4 K) reflection grating spectrometer which operates over the wavelength range from 285 µm–500 µm and was used to post-disperse the output from a room-temperature polarizing FTS. Measurements of the grating resolving power and diffraction efficiency are presented as a function of both wavelength and polarization to characterize the instrument performance
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alicia M. Anderson, David A. Naylor, Brad G. Gom, Ian T. Veenendaal, Adam J. Christiansen, Willem Jellema, and Peter A. R. Ade "Determining the efficiency of a cryogenic far-infrared diffraction grating spectrometer used as a post-dispersing module for a high-resolution spectrometer", Proc. SPIE 12190, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI, 121902C (31 August 2022); https://doi.org/10.1117/12.2628259
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KEYWORDS
Diffraction gratings

Spectroscopy

Fourier transforms

Cryogenics

Spectral resolution

Polarization

Black bodies

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