Development and validation of a cryogenic far-infrared diffraction grating spectrometer used to post-disperse the output from a Fourier transform spectrometer

التفاصيل البيبلوغرافية
العنوان: Development and validation of a cryogenic far-infrared diffraction grating spectrometer used to post-disperse the output from a Fourier transform spectrometer
المؤلفون: Anderson, Alicia M., Naylor, David A., Gom, Brad G., Buchan, Matthew A., Christiansen, Adam J., Veenendaal, Ian T.
المصدر: Rev. Sci. Instrum. 1 January 2024; 95 (1): 015116
سنة النشر: 2024
المجموعة: Astrophysics
Physics (Other)
مصطلحات موضوعية: Physics - Instrumentation and Detectors, Astrophysics - Instrumentation and Methods for Astrophysics
الوصف: 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 diffraction gratings which 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 discusses the development of a cryogenic (4 K) diffraction grating spectrometer which operates over the wavelength range from 285 - 500 $\mu$m and was used to post-disperse the output from a room-temperature polarizing FTS. Measurements of the grating spectral response and diffraction efficiency are presented as a function of both wavelength and polarization to characterize the instrumental performance.
Comment: 9 pages, 14 figures. The following article has been accepted by Review of Scientific Instruments. It can be found at https://doi.org/10.1063/5.0177603
نوع الوثيقة: Working Paper
DOI: 10.1063/5.0177603
URL الوصول: http://arxiv.org/abs/2401.04488
رقم الأكسشن: edsarx.2401.04488
قاعدة البيانات: arXiv