2021 46th International Conference on Infrared, Millimeter and Terahertz Waves (IRMMW-THz) 2021
DOI: 10.1109/irmmw-thz50926.2021.9567358
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Heterodyne Spectroscopy with a 225 – 255 GHz SiGe BiCMOS Receiver for Space Applications

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“…The third important characteristic is the noise performance of the receiver. We were able to determine noise temperatures around 20,000 K, that even allow for passive heterodyne spectroscopy for space applications (see Figure 3) [13]. Furthermore, the RX should have a high dynamic range to allow detection of a wide range of power levels.…”
Section: Tx/rx Characterizationmentioning
confidence: 99%
“…The third important characteristic is the noise performance of the receiver. We were able to determine noise temperatures around 20,000 K, that even allow for passive heterodyne spectroscopy for space applications (see Figure 3) [13]. Furthermore, the RX should have a high dynamic range to allow detection of a wide range of power levels.…”
Section: Tx/rx Characterizationmentioning
confidence: 99%