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Radio interferometer sensitivities for three types of receiving systems: DSB, SSB, and 2SB systems

机译:三种类型的接收系统的无线电干涉仪灵敏度:DSB,SSB和2SB系统

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The purpose of this paper is to study the detection sensitivity suitable to the practical situation for a radio interferometer. For the radio interferometer, the three types of receiving systems are a double-sideband (DSB), a single-sideband (SSB), and a two-single-sideband (2SB) systems. The evaluation of these receiving systems is of significance to explore the best performance for a radio interferometer. In this paper, the signal-to-noise ratios of these three-type receiving systems are newly derived to investigate the performance and key features of each system. We demonstrate the system noise temperatures of SSB, 2SB, and DSB receiving systems by using the ALMA-specification receiver noise temperature and the atmosphere condition measured at the ALMA site, and present the relative sensitivities between the 2SB and DSB receiving systems at the ALMA site. From these results, we recommend the 2SB receiving system for all bands of ALMA.
机译:本文的目的是研究适合无线电干涉仪实际情况的检测灵敏度。对于无线电干涉仪,三种类型的接收系统是双边带(DSB),单边带(SSB)和两单边带(2SB)系统。这些接收系统的评估对于探索无线电干涉仪的最佳性能具有重要意义。在本文中,这三种类型的接收系统的信噪比是新推导的,以研究每个系统的性能和关键特性。我们通过使用ALMA规范的接收器噪声温度和在ALMA站点测量的大气条件来演示SSB,2SB和DSB接收系统的系统噪声温度,并介绍了ALMA站点的2SB和DSB接收系统之间的相对灵敏度。根据这些结果,我们建议对ALMA的所有频段使用2SB接收系统。

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