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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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Betz, A. L., & Borejko, R. T. (1996). A practical Schottky mixer for 5 THz. In Proc. 7th Int. Symp. Space Terahertz Technol. (503).
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Betz, A. L., Boreiko, R. T., Sivananthan, S., & Ashokan, R. (2001). HgCdTe photoconductive mixers for 2-8 THz. In C. Iit.u.t.e of T. Jet Propulsion Laboratory (Ed.), Proc. 12th Int. Symp. Space Terahertz Technol. (pp. 92–101). San Diego, CA, USA.
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Johnson, M. A., Betz, A. L., McLaren, R. A., Townes, C. H., & Sutton, E. C. (1976). Nonthermal 10 micron CO2 emission lines in the atmospheres of Mars and Venus. A&A, 208, 145.
Keywords: carbon dioxide, emission spectra, infrared spectra, mars atmosphere, nonthermal radiation, optical heterodyning, planetary radiation, venus atmosphere, absorption spectra, energy transfer, line spectra, molecular absorption, molecular collisions, near infrared radiation, solar flux
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Betz, A. L., Johnson, M. A., McLaren, R. A., & Sutton, E. C. (1976). Heterodyne detection of CO2 emission lines and wind velocities in the atmosphere of Venus. Astrophys. J., 208, L141–L144.
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Zhou, Y. D., Becker, C. R., Ashokan, R., Selamet, Y., Chang, Y., Boreiko, R. T., et al. (2002). Progress in far-infrared detection technology. In Proc. SPIE (Vol. 4795, pp. 121–128). Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series.
Abstract: II-VI intrinsic very long wavelength infrared (VLWIR, λc~20 to 50 μm) materials, HgCdTe alloys as well as HgCdTe/CdTe superlattices, were grown by molecular beam epitaxy (MBE). The layers were characterized by means of X-ray diffraction, conventional Fourier transform infrared spectroscopy, Hall effect measurements and transmittance electron microscopy (TEM). Photoconductor devices were processed and their spectral response was also measured to demonstrate their applicability in the VLWIR region.
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