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MEGARA MOS:where are my positioners and fibers pointing to?

机译:MEGARA MOS:我的定位器和光纤指向哪里?

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MEGARA is an integral-field and multi-object medium-resolution spectrograph for the GTC 10.4m telescope, which was commissioned on June - August 2017. MEGARA offers two observing modes, the LCB mode, a large central IFU; and a Multi-Object Spectrograph (MOS) mode, composed by 92 robotic positioners carrying 7-fiber minibundles each. This paper presents the models and measurements developed for the alignment between the image of the telescope pupil and the 100-μm fiber cores during the integration and verification at the laboratory. On the one hand, the error in the positioner-minibundles assembly was optimized with the aim of achieving a fiber-to-fiber flux homogeneity better than 10%. On the other hand, the positioner pointing was characterized in order to achieve a pointing precision of 1/5 of the spaxel size (which has been designed to be 0.62 arcsec). The on-sky measurements obtained during the commissioning to verify our laboratory results are also presented.
机译:MEGARA是GTC 10.4m望远镜的积分场和多对象中分辨率光谱仪,已于2017年6月-2017年8月投入使用。MEGARA提供两种观测模式:LCB模式,大型中央IFU。还有一个多目标光谱仪(MOS)模式,该模式由92个机器人定位器组成,每个定位器均带有7根光纤微型束。本文介绍了在实验室集成和验证过程中为望远镜瞳孔图像和100-μm光纤纤芯之间的对准而开发的模型和测量结果。一方面,优化了定位器-微束组件中的误差,目的是使光纤间的通量均匀性好于10%。另一方面,定位器定位的特点是达到Spaxel大小(设计为0.62 arcsec)的1/5的定位精度。还介绍了在调试过程中获得的空中测量结果,以验证我们的实验室结果。

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