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Alignment of the SPHERE-ZIMPOL imaging polarimeter

机译:SPHERE-ZIMPOL成像旋光仪的对准

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ZIMPOL is the high contrast imaging polarimeter subsystem of the ESO SPHERE instrument. ZIMPOL is dedicated todetect the very faint reflected and hence polarized visible light from extrasolar planets. ZIMPOL is located behind anextreme AO system (SAXO) and a stellar coronagraph. SPHERE is foreseen to have first light at the VLT early 2013.ZIMPOL is currently integrated in the SPHERE system and in testing phase.We describe the alignment strategy and the results of the ZIMPOL system and the related alignment of ZIMPOL intoSPHERE by the aid of an alignment unit. The field selecting tip/tilt mirror alignment and it’s requirement forperpendicularity to the two detectors is described. The test setup of the polarimetric components is described.SPHERE is an instrument designed and built by a consortium consisting of IPAG, MPIA, LAM, LESIA, Fizeau, INAF,Observatoire de Genève, ETH, NOVA, ONERA and ASTRON in collaboration with ESO.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:ZIMPOL是ESO SPHERE仪器的高对比度成像旋光仪子系统。 ZIMPOL致力于探测来自太阳系外行星的非常微弱的反射光和偏振光。 ZIMPOL位于极端AO系统(SAXO)和恒星日冕仪的后面。预计SPHERE将于2013年初在VLT上首次亮相。目前,ZIMPOL已集成到SPHERE系统和测试阶段。对齐单元。描述了选择倾斜/倾斜镜对准的场及其对两个探测器的垂直性要求。描述了极化组件的测试设置。SPHERE是由IPAG,MPIA,LAM,LESIA,Fizeau,INAF,日内瓦观察站,ETH,NOVA,ONERA和ASTRON与ESO合作组成的财团设计和制造的仪器。 ©(2012)版权所有,光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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