Development of 1.25 THz SIS mixer for Herschel Space Observatory

Abstract

ABSTRACT We summarize the development and the delivery of two SIS mixers for the 1.1-1.25 THz band of the heterodyne spectrometer of Herschel Observatory (HSO). The quasi-op tical SIS mixer has two Nb/Al N/NbTiN junctions with the area of 0.25 um 2 . The Josephson critical current density in the junction is 30-50 kA/cm . The tuning circuit integrated with SIS junc tion has the base electrode of Nb and a gold wire layer. With the new SIS mixers the test receiver maximum Y factor is 1.41. The minimum receiver uncorrected DSB noise temperature is 450 K. The SIS receiver noise corrected for the loss in the optics is 350-450 K across the 1100-1250 GHz band. The receiver has a uniform sensitivity in the full IF range of 4-8 GHz. The sub-micron sized SIS junction shape is optimized to ease the suppression of the Josephson current, and the receiver operation is stable. The measured mixer beam pattern is symmetrical and, in a good agreement with the requirements, has the f/d =4.25 at the central frequency of the operation band. The minimum DSB SIS receiver noise is close to 6 hv/k, the lowest value achieved thus far in the THz frequencies range. Keywords: SIS mixer, THz frequency, far infrared, low noise, Herschel space observatory, radio astronomy.