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首页> 外文会议>Conference on ground-based and airborne instrumentation for astronomy IV >Hector: a high-multiplex survey instrument for spatially resolved galaxy spectroscopy
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Hector: a high-multiplex survey instrument for spatially resolved galaxy spectroscopy

机译：赫克托（Hector）：一种用于空间分辨星系光谱学的高倍调查仪器

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First light from the SAMI (Sydney-AAO Multi-object IFS) instrument at the Anglo-Australian Telescope (AAT) hasrecently proven the viability of fibre hexabundles for multi-IFU spectroscopy. SAMI, which comprises 13 hexabundleIFUs deployable over a 1 degree field-of-view, has recently begun science observations, and will target a survey ofseveral thousand galaxies. The scientific outputs from such galaxy surveys are strongly linked to survey size, leading thepush towards instruments with higher multiplex capability. We have begun work on a new instrument concept, calledHector, which will target a spatially-resolved spectroscopic survey of up to one hundred thousand galaxies. The keyscience questions for this instrument concept include how do galaxies get their gas, how is star formation and nuclearactivity affected by environment, what is the role of feedback, and what processes can be linked to galaxy groups andclusters. One design option for Hector uses the existing 2 degree field-of view top end at the AAT, with 50 individualrobotically deployable 61-core hexabundle IFUs, and 3 fixed format spectrographs covering the visible wavelength rangewith a spectral resolution of approximately 4000. A more ambitious option incorporates a modified top end at the AATwith a new 3 degree field-of-view wide-field-corrector and 100 hexabundle IFUs feeding 6 spectrographs.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译：英澳望远镜（AAT）的SAMI（悉尼-AAO多目标IFS）仪器的第一束光最近证明了用于多IFU光谱的纤维六束纤维的可行性。 SAMI由13个hexabundleIFU组成，可在1度视场内部署，最近已开始进行科学观测，并将针对数千个星系进行调查。此类银河系测量的科学输出与测量规模紧密相关，从而将推力推向了具有更高复用能力的仪器。我们已经开始研究一种名为赫克托（Hector）的新仪器概念，该仪器的目标是对多达十万个星系进行空间分辨光谱学调查。该仪器概念的关键科学问题包括：星系如何获取气体，星际形成和核活动如何受到环境的影响，反馈的作用是什么以及哪些过程可以与星系和团簇联系在一起。赫克托的一种设计选择是使用AAT处现有的2度视野顶端，以及50个可机器人部署的61芯六束IFU，以及3个固定格式的光谱仪，其光谱范围约为4000，可见光谱范围更广。该选件在AAT处集成了改进的顶端，带有一个新的3度视野广域校正器和100个六束IFU，可为6个光谱仪供能。©（2012）COPYRIGHT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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