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The imaging and slitless spectroscopy instrument for surveys (ISSIS) for the world space observatory-ultraviolet (WSO-UV)

机译:用于世界空间天文台-紫外线(WSO-UV)的成像成像和无狭缝光谱调查仪器(ISSIS)

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摘要

ISSIS is the Imaging and Slitless Spectroscopy Instrument for the World Space Observatory-Ultraviolet (WSO-UV) mission. ISSIS is a multipurpose instrument designed to carry out high resolution (<0. 1 arcsec) imaging in the far UV with fields of view ≥2×2 arcmin~2. ISSIS has two acquisition channels: the High Sensitivity Channel (HSC) and the Channel for Surveys (CfS). The HSC is equipped with an MCP-type detector to guarantee high sensitivity in the 1150-1750 ? range and high rejection of lower energy radiation. The CfS is equipped with a large CCD detector (4k×4k) to obtain images from the far UV to the red (1150-8500 ?); the CfS is implemented to allow observing UV bright sources such as reflection nebulae or nearby massive star forming regions. The design drivers and the current status of the instrument are described in this contribution.
机译:ISSIS是用于执行世界空间天文台-紫外线(WSO-UV)任务的成像和无缝光谱仪。 ISSIS是一种多功能仪器,设计用于在远场UV中以≥2×2 arcmin〜2的视场进行高分辨率(<0.1弧秒)成像。 ISSIS具有两个采集通道:高灵敏度通道(HSC)和调查通道(CfS)。 HSC配备了MCP型检测器,以确保在1150-1750?范围和对低能量辐射的高抑制。 CfS配备了一个大型CCD检测器(4k×4k),以获取从远紫外线到红色(1150-8500?)的图像;执行CfS的目的是允许观察UV亮源,例如反射星云或附近的大质量恒星形成区域。本文稿介绍了设计驱动程序和仪器的当前状态。

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