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Semenov AD, Hübers H-W, Richter H, Birk M, Krocka M, Mair U, et al. 2.5 THz heterodyne receiver with NbN hot-electron-bolometer mixer. Phys C: Supercond. 2002;372-376:448–53.
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Lindgren M, Currie M, Zeng W-S, Sobolewski R, Cherednichenko S, Voronov B, et al. Picosecond response of a superconducting hot-electron NbN photodetector. Appl Supercond. 1998;6(7-9):423–8.
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Gol'tsman GN. Hot electron bolometric mixers: new terahertz technology. Infrared Physics & Technology. 1999;40(3):199–206.
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Kitaygorsky J, Komissarov I, Jukna A, Minaeva O, Kaurova N, Divochiy A, et al. Fluctuations in two-dimensional superconducting NbN nanobridges and nanostructures meanders [abstract]. In: Proc. APS March Meeting. Vol 52.; 2007. L9.00013.
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Boyarskii DA, Gershenzon VE, Gershenzon EM, Gol'tsman GN, Ptitsina NG, Tikhonov VV, et al. On the possibility of determining the microstructural parameters of an oil-bearing layer from radiophysical measurement data. J of Communications Technology and Electronics. 1996;41(5):408–14.
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Gao JR, Hajenius M, Baselmans JJA, Klapwijk TM, de Korte PAJ, Voronov B, et al. NbN hot electron bolometer mixers with superior performance for space applications. In: Armandillo E, Leone B, editors. Proc. Int. workshop on low temp. electronics. Noordwijk; 2004. p. 11–7.
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Gershenson EM, Gol'tsman GN, Elant'ev AI, Kagane ML, Multanovskii VV, Ptitsina NG. Use of submillimeter backward-wave tube spectroscopy in determination of the chemical nature and concentration of residual impurities in pure semiconductors. Sov Phys Semicond. 1983;17(8):908–13.
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Gershenzon EM, Gol'tsman GN. Effect of electromagnetic radiation on a superconductor in a magnetic field. In: Izv. Akad. Nauk SSSR, Seriya Fizicheskaya. Vol 52.; 1988. p. 449–51.
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Karasik BS, Il'in KS, Ptitsina NG, Gol'tsman GN, Gershenzon EM, Pechen' EV, et al. Electron-phonon scattering rate in impure NbC films [abstract]. In: NASA/ADS.; 1998. Y35.08.
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Hübers H-W, Semenov A, Richter H, Smirnov K, Gol'tsman G, Voronov B. Phonon cooled far-infrared hot electron bolometer mixer [abstract]. In: NASA/ADS.; 2002.
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