Abstract
A waveguide SIS heterodyne receiver using a Nb/AlOX/Nb junction has been built for astronomical observations of molecular transitions in the frequency range 600 GHz - 635 GHz, and has been successfully used at the Caltech Submillimeter Observatory (CSO). We report double sideband (DSB) receiver noise temperatures as low as 245 K at 600 GHz -610 GHz, and near 300 K over the rest of the bandwidth. These results confirm that SIS quasiparticle mixers work well at submillimeter-wave frequencies corresponding to photon energies of at least 90% of the superconductor energy gap. In addition, we have systematically investigated the effect on the receiver performance of the overlap between first-order and second-order photon steps of opposite sign at these frequencies. The receiver noise increases by as much as 40% in the region of overlap. We infer potential limitations for operating submillimeter-wave Nb/AlOx/Nb mixers.
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Salez, M., Febvre, P., Mcgrath, W.R. et al. An SIS waveguide heterodyne receiver for 600 HGz-635 GHz. Int J Infrared Milli Waves 15, 349–368 (1994). https://doi.org/10.1007/BF02096246
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DOI: https://doi.org/10.1007/BF02096246