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Piotr슠Orleanski, Miroslaw슠Ciechanowicz, Malgorzata슠Michalska, Witold슠Nowosielski, Miroslaw슠Rataj, Marek슠Winkler. LCU: the control unit dedicated for local oscillator subsystem in ESA HIFI/Herschel project. In: Proc. SPIE. Vol 6159.; 2006.
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de Graauw T, Whyborn N, Caux E, Phillips T, Stutzki J, Tielens X, et al. The Herschel-heterodyne instrument for the far-infrared (HIFI). In: Proc. SPIE. Orlando; 2006.
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Thijs de Graauw, Nick Whyborn, Frank Helmich, Pieter Dieleman, Peter Roelfsema, Emmanuel Caux, et al. The Herschel-heterodyne instrument for the far-infrared (HIFI): instrument and pre-launch testing. In: Proc. SPIE. Vol 7010.; 2008. 701004.
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Gol'tsman GN, Vachtomin YB, Antipov SV, Finkel MI, Maslennikov SN, Smirnov KV, et al. NbN phonon-cooled hot-electron bolometer mixer for terahertz heterodyne receivers. In: Proc. SPIE. Vol 5727.; 2005. p. 95–106.
Abstract: We present the results of our studies of NbN phonon-cooled HEB mixers at terahertz frequencies. The mixers were fabricated from NbN film deposited on a high-resistivity Si substrate with an MgO buffer layer. The mixer element was integrated with a log-periodic spiral antenna. The noise temperature measurements were performed at 2.5 THz and at 3.8 THz local oscillator frequencies for the 3 x 0.2 μm2 active area devices. The best uncorrected receiver noise temperatures found for these frequencies are 1300 K and 3100 K, respectively. A water vapour discharge laser was used as the LO source. The largest gain bandwidth of 5.2 GHz was achieved for a mixer based on 2 nm thick NbN film deposited on MgO layer over Si substrate. The gain bandwidth of the mixer based on 3.5 nm NbN film deposited on Si with MgO is 4.2 GHz and the noise bandwidth for the same device amounts to 5 GHz. We also present the results of our research into decrease of the direct detection contribution to the measured Y-factor and a possible error of noise temperature calculation. The use of a square nickel cell mesh as an IR-filter enabled us to avoid the effect of direct detection and measure apparent value of the noise temperature which was 16% less than that obtained using conventional black polyethylene IR-filter.
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David Olaya, Jian Wei, Sergei Pereverzev, Karasik BS, Kawamura Jhan H, McGrath WR, et al. An ultrasensitive hot-electron bolometer for low-background SMM applications. In: Proc. SPIE. Vol 6275.; 2006. 627506.
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Karpov A, Miller D, Rice F, Stern JA, Bumble B, LeDuc HG, et al. Development of 1.25 THz SIS mixer for Herschel Space Observatory. In: Zmuidzinas J, Holland WS, editors. Proc. SPIE. Vol 6275.; 2006. 62751.
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Brown RL. Technical specification of the Millimeter Array. In: Phillips TG, editor. Proc. SPIE, Advanced Technology MMW, Radio, and Terahertz Telescopes, vol. 3357.; 1998. p. 231–7.
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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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Amato MJ, Benford DJ, Moseley HS, Juan Roman. An engineering concept and enabling technologies for a large single aperture far-infrared observatory (SAFIR). In: Proc. SPIE. Vol 4850.; 2003. p. 1120–31.
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Yorke HW, Paine CG, Bradford CM, Mark Dragovan, Nash AE, Dooley JA, et al. Thermal design trades for SAFIR architecture concepts. In: Proc. SPIE. Vol 5487.; 2004. p. 1617–24.
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