Design and Fabrication Highlights Enabling a 2 mm, 128 Element Bolometer Array for GISMO
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Abstract
The Backshort-Under-Grid (BUG) superconducting bolometer array architecture is intended to be highly versatile, operating over a large range of wavelengths and background conditions. To validate the basic array design and to demonstrate its applicability for future kilopixel arrays, we will demonstrate a 128-element bolometer array optimized for 2 mm wavelength using a new Goddard Space Flight Center instrument, GISMO (Goddard IRAM Superconducting 2-Millimeter Observer). The design considerations unique to GISMO and laboratory experimental results will be discussed.
Keywords
Bolometer array Transition edge sensorPACS
07.57.Kp 95.55.Rg 85.25.-jPreview
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