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  • 1
    Publication Date: 2019-07-13
    Description: Micro-Spec (-Spec) is a direct-detection spectrometer which integrates all the components of a diffraction-grating spectrometer onto a 10-cm2 chip through the use of superconducting microstrip transmission lines on a single-crystal silicon substrate. A second-generation -Spec is being designed to operate with a spectral resolution of 512 in the submillimeter (500-1000 m, 300-600 GHz) wavelength range, a band of interest for several spectroscopic applications in astrophysics. High altitude balloon missions would provide the first test bed to demonstrate the -Spec technology in a space-like environment and would be an economically viable venue for multiple observation campaigns. This work reports on the current status of the instrument design and will provide a brief overview of each instrument subsystem. Particular emphasis will be given to the design of the spectrometer's two-dimensional diffractive region, through which the light of different wavelengths is focused on the detectors along the focal plane. An optimization process is employed to generate geometrical configurations of the diffractive region that satisfy specific requirements on spectrometer size, operating spectral range, and performance. An optical design optimized for balloon missions will be presented in terms of geometric layout, spectral purity, and efficiency.
    Keywords: Instrumentation and Photography
    Type: GSFC-E-DAA-TN58545 , Journal of Low Temperature Physics (ISSN 0022-2291) (e-ISSN 1573-7357); 1-8
    Format: text
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  • 2
    Publication Date: 2019-09-27
    Description: The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) is a cryogenic balloon-borne instrument which will survey galaxy and star formation history over cosmological time scales. Rather than identifying individual objects, EXCLAIM will be a pathfinder to demonstrate an intensity mapping approach, which measures the cumulative redshifted line emission. EXCLAIM will operate at 420-540 GHz with a spectral resolution R=512 to measure the integrated CO and [CII] in redshift windows spanning \exclaimz. CO and [CII] line emissions are key tracers of the gas phases in the interstellar medium involved in star-formation processes. EXCLAIM will shed light on questions such as why the star formation rate declines at z 〈 2, despite continued clustering of the dark matter. The instrument will employ an array of six superconducting integrated grating-analog spectrometers (-Spec) coupled to microwave kinetic inductance detectors (MKIDs). Here we present an overview of the EXCLAIM instrument design and status.
    Keywords: Astrophysics; Instrumentation and Photography
    Type: GSFC-E-DAA-TN73265 , International Workshop on Low Temperature Detectors; Jul 22, 2019 - Jul 26, 2019; Milan; Italy
    Format: application/pdf
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