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Burke, P. J., Schoelkopf, R. J., Prober, D. E., Skalare, A., Karasik, B. S., Gaidis, M. C., et al. (1999). Mixing and noise in diffusion and phonon cooled superconducting hot-electron bolometers. J. Appl. Phys., 85(3), 1644–1653.
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Mason, W., & Waterman, J. R. (1999). Electrical and optical characteristics of two color mid wave HgCdTe infrared detectors. Appl. Phys. Lett., 74(11), 1633–1635.
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Kawamura, J., Blundell, R., Tong, C. -yu E., Gol’tsman, G., Gershenzon, E., Voronov, B., et al. (1997). Low noise NbN lattice-cooled superconducting hot-electron bolometric mixers at submillimeter wavelengths. Appl. Phys. Lett., 70(12), 1619–1621.
Abstract: Lattice-cooled superconducting hot-electron bolometric mixers are used in a submillimeter-wave waveguide heterodyne receiver. The mixer elements are niobium nitride film with 3.5 nm thickness and ∼10 μm2 area. The local oscillator power for optimal performance is estimated to be 0.5 μW, and the instantaneous bandwidth is 2.2 GHz. At an intermediate frequency centered at 1.4 GHz with 200 MHz bandwidth, the double sideband receiver noise temperature is 410 K at 430 GHz. The receiver has been used to detect molecular line emission in a laboratory gas cell.
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Johnson, M. A., Betz, A. L., & Townes, C. H. (1974). 10-μm Heterodyne Stellar Interferometer. Phys. Rev. Lett., 33(27), 1617–1620.
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Yorke, H. W., Paine, C. G., Bradford, C. M., Mark Dragovan, Nash, A. E., Dooley, J. A., et al. (2004). Thermal design trades for SAFIR architecture concepts. In Proc. SPIE (Vol. 5487, pp. 1617–1624).
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