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Gol'tsman GN, Loudkov DN. Terahertz superconducting hot-electron bolometer mixers and their application in radio astronomy. Radiophys. Quant. Electron.. 2003;46(8/9):604–17.
Abstract: We review the latest developments, research, and radioastronomy applications of hot-electron bolometer (HEB) mixers operated in the terahertz waveband. The physical principles of operation of terahertz HEB mixers are presented, their manufacturing from ultrathin NbN films, the main HEB-mixer parameters and their measurement techniques are discussed, and practical terahertz radioastronomy projects based on heterodyne receivers with HEB mixers are considered.
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Zhang J, Boiadjieva N, Chulkova G, Deslandes H, Gol'tsman GN, Korneev A, et al. Noninvasive CMOS circuit testing with NbN superconducting single-photon detectors. Electron Lett. 2003;39(14):1086–8.
Abstract: The 3.5 nm thick-film, meander-structured NbN superconducting single-photon detectors have been implemented in the CMOS circuit-testing system based on the detection of near-infrared photon emission from switching transistors and have significantly improved the performance of the system. Photon emissions from both p- and n-MOS transistors have been observed.
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Zwiller V, Aichele T, Seifert W, Persson J, Benson O. Generating visible single photons on demand with single InP quantum dots. Appl Phys Lett. 2003;82(10):1509–11.
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Benford DJ, Gaidis MC, Kooi JW. Optical properties of Zitex in the infrared to submillimeter. Appl Opt. 2003;42(25):5118.
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Kostiuk T. Heterodyne spectroscopy in the thermal infrared region: a window on physics and chemistry. In: University of Maryland Inn and Conference Center, editor. Proc. International Thermal Detectors Workshop (TDW'03), session 7 (Heterodyne detectors). 3501 University Boulevar East Adelphi, MD 20783; 2003.
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Snyder Hale DD. A thermal infrared heterodyne receiver with applications to astronomy. Berkeley, CA 94720; 2003.
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Stéphane Claude. Sideband-separating SIS mixer for ALMA band 7, 275–370 GHz. In: Proc. 14th Int. Symp. Space Terahertz Technol. Tucson, USA; 2003. 41.
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Grimes P, Kittara P, Yassin G, Withington S, Jacobs K. Investigation of the performance of a 700 GHz nline mixer. In: Proc. 14th Int. Symp. Space Terahertz Technol. Tucson, USA; 2003. 247.
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Huebers H-W, Semenov A, Richter H, Birk M, Krocka M, Mair U, et al. Superconducting hot electron bolometer as mixer for far-infrared heterodyne receivers. In: Phillips TG, Zmuidzinas J, editors. Proc. SPIE. Vol 4855. Tucson, USA: SPIE; 2003. p. 395–401. (Presented at the Society of Photo-Optical Instrumentation Engineers (SPIE) Conference; vol 4855).
Abstract: Heterodyne receivers for applications in astronomy need quantum limited sensitivity. In instruments which are currently under development for SOFIA or Herschel superconducting hot electron bolometers (HEB) will be used to achieve this goal at frequencies above 1.4 THz. We present results of the development of a phonon-cooled NbN HEB mixer for GREAT, the German Receiver for Astronomy at Terahertz Frequencies, which will be flown aboard SOFIA. The mixer is a small superconducting bridge incorporated in a planar feed antenna and a hyperhemispherical lens. Mixers with logarithmic-spiral and double-slot feed antennas have been investigated with respect to their noise temperature, conversion loss, linearity and beam pattern. At 2.5 THz a double sideband noise temperature of 2200 K was achieved. The conversion loss was 17 dB. The response of the mixer was linear up to 400 K load temperature. The performance was verified by measuring an emission line of methanol at 2.5 THz. The measured linewidth is in good agreement with the linewidth deduced from pressure broadening measurements at millimeter wavelength. The results demonstrate that the NbN HEB is very well suited as a mixer for far-infrared heterodyne receivers.
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Hajenius M, Baselmans JJA, Gao JR, Klapwijk TM, de Korte PAJ, Voronov B, et al. Improved NbN phonon cooled hot electron bolometer mixers. In: Proc. 14th Int. Symp. Space Terahertz Technol. Tucson, USA; 2003. p. 413–23.
Abstract: NbN phonon-cooled hot electron bolometer mixers (HEBs) have been realized with negligible contact resistance to Au pads. By adding either a 5 nm Nb or a 10 nm NbTiN layer between the Au and NbN, to preserve superconductivity in the NbN under the Au contact pad, superior noise temperatures have been obtained. Using DC I,V curves and resistive transitions in combination with process parameters we analyze the nature of these improved devices and determine interface transparencies.
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