Shafinaz Ali,1 Peter T. Timbie,1 Siddharth Malu,1 Dan McCammon,1 Kari L. Nelms,1 Rashmi Pathak,1 Daniel W. van der Weide,1 Christine A. Allen,2 J. Abrahams,2 James A. Chervenak,2 Wen-Ting Hsieh,2 Timothy M. Miller,2 S. Harvey Moseley Jr.,2 Thomas R. Stevenson,2 Edward J. Wollackhttps://orcid.org/0000-0002-7567-44512
1Univ. of Wisconsin/Madison (United States) 2NASA Goddard Space Flight Ctr. (United States)
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We are developing a new type of detector for observational cosmology and astrophysical research. Incoming radiation from the sky is coupled to a superconducting microstrip transmission line that terminates in a thin film absorber. At sub-Kelvin temperature, the thermal isolation between the electrons and the lattice makes it possible for the electrons in the small absorber (100's of cubic micro-meter) and superconducting bilayer (Transition Edge Sensor) to heat up by the radiation absorbed by the electrons of the normal absorbing layer. We call this detector a Transition-edge Hot-electron Micro-bolometer (THM). THMs can be fabricated by photo lithography, so it is relatively easy to make matched detectors for a large focal plane array telescope. We report on the thermal properties of Mo/Au THMs with Bi/Au absorbers.
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Shafinaz Ali, Peter T. Timbie, Siddharth Malu, Dan McCammon, Kari L. Nelms, Rashmi Pathak, Daniel W. van der Weide, Christine A. Allen, J. Abrahams, James A. Chervenak, Wen-Ting Hsieh, Timothy M. Miller, S. Harvey Moseley Jr., Thomas R. Stevenson, Edward J. Wollack, "Antenna-coupled transition-edge hot-electron microbolometers," Proc. SPIE 5498, Millimeter and Submillimeter Detectors for Astronomy II, (8 October 2004); https://doi.org/10.1117/12.552836