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Antipov SV, Svechnikov SI, Smirnov KV, Vakhtomin YB, Finkel MI, Goltsman GN, et al. Noise temperature of quasioptical NbN hot electron bolometer mixers at 900 GHz. Physics of Vibrations. 2001;9(4):242–5.
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Svechnikov SI, Antipov SV, Vakhtomin YB, Goltsman GN, Gershenzon EM, Cherednichenko SI, et al. Conversion and noise bandwidths of terahertz NbN hot-electron bolometer mixers. Physics of Vibrations. 2001;9(3):205–10.
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Verevkin AA, Ptitsina NG, Smirnov KV, Goltsman GN, Gershenson EM, Yngvesson KS. Direct measurements of electron energy relaxation times at an AlGaAs/GaAs heterointerface in the optical phonon scattering range. In: Proc. 4-th Int. Semicond. Device Research Symp.; 1997. p. 55–8.
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Ekström H, Kroug M, Belitsky V, Kollberg E, Olsson H, Goltsman G, et al. Hot electron mixers for THz applications. In: Rolfe EJ, Pilbratt G, editors. Proc. 30th ESLAB.; 1996. p. 207–10.
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Kollberg EL, Gershenzon E, Goltsman G, Yngvesson KS. Hot electron mixers, the potential competition. In: Proc. ESA Symp. on Photon Detectors for Space Instrumentation.; 1992. p. 201–6.
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Gershenzon EM, Gogidze IG, Goltsman GN, Semenov AD, Sergeev AV. Picosecond response on optical-range emission in thin YBaCuO films. Pisma v Zhurnal Tekhnicheskoi Fiziki. 1991;17(22):6–10.
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Voevodin EI, Gershenzon EM, Goltsman GN, Ptitsina NG. Energy-spectrum of shallow acceptors in Ge deformed strongly by a uniaxial pressure. Sov Phys and Technics of Semiconductors. 1989;23(8):843–6.
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Aksaev EE, Gershenzon EM, Gershenson ME, Goltsman GN, Semenov AD, Sergeev AV. Prospects for using high-temperature superconductors to create electron bolometers. Pisma v Zhurnal Tekhnicheskoi Fiziki. 1989;15(14):88–93.
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Gershenzon EM, Gershenson ME, Goltsman GN, Karasik BS, Lyulkin AM, Semenov AD. Fast-response superconducting electron bolometer. Pisma v Zhurnal Tekhnicheskoi Fiziki. 1989;15(3):88–92.
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Gershenzon EM, Gershenson ME, Goltsman GN, Lyulkin AM, Semenov AD, Sergeev AV. Limiting characteristics of fast-response superconducting bolometers. Zhurnal Tekhnicheskoi Fiziki. 1989;59(2):11–120.
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