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The QUIJOTE TGI

机译:QUIXOTE TGI

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摘要

The QUIJOTE TGI instrument is currently being assembled and tested at the IAC in Spain. The TGI is a 31 pixel 26-36 GHz polarimeter array designed to be mounted at the focus of the second QUIJOTE telescope. This follows a first telescope and multi-frequency instrument that have now been observing almost 2 years. The polarimeter design is based on the QUIET polarimeter scheme but with the addition of an extra 90° phase switch which allows for quasi-instantaneous complete QUI measurements through each detector. The advantage of this is a reduction in the systematics associated with differencing two independent radiometer channels. The polarimeters are split into a cold front end and a warm back end. The back end is a highly integrated design by engineers at DICOM. It is also sufficiently modular for testing purposes. In this presentation the high quality wide band components used in the optical design (also designed in DICOM) are presented as well as the novel cryogenic modular design. Each polarimeter chain is accessible individually and can be removed from the cryostat and replaced without having to move the remaining pixels. The optical components work over the complete Ka band showing excellent performance. Results from the sub unit measurements are presented and also a description of the novel calibration technique that allows for bandpass measurement and polar alignment. Terrestrial Calibration for this instrument is very important and will be carried out at three points in the commissioning phase: in the laboratory, at the telescope site and finally a reduce set of calibrations will be carried out on the telescope before measurements of extraterrestrial sources begin. The telescope pointing model is known to be more precise than the expected calibration precision so no further significant error will be added through the telescope optics. The integrated back-end components are presented showing the overall arrangement for mounting on the cryostat. Many of the microwave circuits are in-house designs with performances that go beyond commercially available products. Individual component performance is be presented showing for each of the sub modules
机译:QUIJOTE TGI仪器目前正在西班牙的IAC进行组装和测试。 TGI是一个31像素的26-36 GHz偏振计阵列,旨在安装在第二台QUIJOTE望远镜的焦点处。在此之前,第一台望远镜和多频仪器已经观测了近两年。旋光仪的设计基于QUIET旋光仪方案,但增加了一个额外的90°相位开关,该开关允许通过每个检测器进行准瞬时完整的QUI测量。这样做的好处是减少了与两个独立的辐射计通道的差分相关的系统。旋光仪分为冷前端和热后端。后端是DICOM工程师的高度集成设计。它也足够模块化以用于测试目的。在本演示中,将介绍光学设计(也在DICOM中进行设计)中使用的高质量宽带组件以及新颖的低温模块化设计。每个旋光仪链都可以单独访问,并且可以从低温恒温器中取出并更换,而无需移动其余像素。光学元件在整个Ka波段上工作,表现出出色的性能。给出了子单元测量的结果,并介绍了允许带通测量和极性对准的新型校准技术。该仪器的地面校准非常重要,将在调试阶段的三个点进行:在实验室的望远镜现场,最后在开始测量地外源之前,将在望远镜上进行一系列简化的校准。众所周知,望远镜指向模型比预期的校准精度更为精确,因此不会通过望远镜光学系统进一步增加重大误差。展示了集成的后端组件,显示了安装在低温恒温器上的总体布置。许多微波电路是内部设计,其性能超出了市售产品。呈现了单个组件的性能,显示了每个子模块的性能

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