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345 GHZ PROTOTYPE SIS MIXER WITH INTEGRATED MMIC LNA |
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| Authors: | P Pütz A Hedden P Gensheimer D Golish C E Groppi C Kulesa G Narayanan A Lichtenberger J W Kooi N Wadefalk S Weinreb and C K Walker |
| Institution: | (1) Steward Observatory, University of Arizona, Tucson, AZ 85721, USA;(2) KOSMA, I. Phys. Institut, Universit?t zu K?ln, 50937 K?ln, Germany;(3) Astronomy Dep., University of Massachusetts, Amherst, MA 01003, USA;(4) ECE Dep., University of Virginia, Charlottesville, VA 22904, USA;(5) Caltech, MS 320-47, Pasadena, CA 91125, USA;(6) Caltech, MS 136-93, Pasadena, CA 91125, USA |
| Abstract: | We report on heterodyne measurements at submillimeter wavelengths using a receiver with a Superconductor-Insulator-Superconductor (SIS) mixer device and a Microwave Monolithic Integrated Circuit (MMIC) cryogenic low noise amplifier (LNA) module integrated into the same block. The mixer characterization presented in this work demonstrates the feasibility of operating a MMIC LNA in close proximity to the SIS device without penalty in mixer performance due to heating effects. Verification of this functionality is crucial for the ongoing development of SuperCam, a 64-pixel focal plane array receiver consisting of eight, 1 × 8 integrated mixer/LNA modules. The test setup included a mixer block modified to accept a MMIC amplifier. Our tests show that the LNA can be operated over a broad range of Vdrain voltages from 0.40–1.40 V, corresponding to dissipative powers of 2.6–29 mW. We observe no significant effect on the measured uncorrected receiver noise temperatures in the 345 GHz band. |
| Keywords: | submillimeter heterodyne receiver SIS mixer MMIC low noise amplifier array |
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