Deployment of a fully integrated 360GHz Schottky Diode Based Receiver at the Mexican Large Millimetre Telescope

N.S. Daghestani, F. Cahill, A. Obeed, E. Gallagher,E. Colin-Beltran, D. Sanchez-Arguelles,Stan Kurtz, D. Hughes,G. A. Fuller,M. Dunstan,S. Parkes,B.N. Ellison

2020 45th International Conference on Infrared, Millimeter, and Terahertz Waves (IRMMW-THz)(2020)

引用 0|浏览0
暂无评分
摘要
A room temperature sub-millimetre-wave Schottky barrier diode heterodyne receiver system (the Collaborative Heterodyne Astronomical Receiver for Mexico aka CHARM) operating at ~360GHz, has been deployed at the Large Millimetre Telescope, Mexico. The receiver is fully integrated as a turn-key system, and uses a double-sideband subharmonic mixer with an average noise equivalent system temperature of 1,000K. The system back-end signal processing incorporates four wide-band digital spectrometers, with a combined instantaneous IF bandwidth of 10.4GHz for both upper and lower side-bands, and a channel spectral resolution of 1.2MHz. The system has been used to observe first light with the LMT in the sub-millimetre-wave range. It will be further used to perform estimates of the telescope system performance in support of future sub-millimetre-wave observations from the LMT.
更多
查看译文
关键词
fully integrated 360GHz Schottky diode,Collaborative Heterodyne Astronomical Receiver,Mexico aka CHARM,double-sideband subharmonic mixer,average noise equivalent system temperature,wide-band digital spectrometers,sub-millimetre-wave range,telescope system performance,sub-millimetre-wave observations,Mexican Large Millimetre Telescope,submillimetre-wave Schottky barrier diode heterodyne receiver system,frequency 1.2 MHz,frequency 360.0 GHz,temperature 293.0 K to 298.0 K,temperature 1.0 K,frequency 10.4 GHz
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要