Indian spectroscopic and imaging space telescope (INSIST): An optics design trade-off study

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
S. Sriram, Vineeth Valsan, A. Subramaniam, C. Vishnu Unni, G. Maheswar, Totan Chand
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Abstract

Large ground and space-based surveys in optical and near-infrared (NIR) wavelengths will revolutionize astronomy in the coming decade. Unfortunately, no ultraviolet (UV) facilities are planned to complement these surveys, which is crucial for studying the most active phase of the Universe that includes star formation in galaxies, active galactic nuclei (AGN), galaxy clusters, etc. A dedicated UV mission, the Indian Spectroscopic and Imaging Space Telescope (INSIST), is proposed to observe the UV sky. The compelling science objectives defined a set of high-level mission requirements. According to which, the INSIST is to have a wide field-of-view (\(\textrm{FoV} \approx 0.25\) square degree) comparable to India’s Ultraviolet Imaging Telescope (UVIT) and about two orders of magnitude larger than that of the Hubble Space Telescope, simultaneous imaging of the FoV in UV (150–300 nm), u (300–400 nm) and g (400–550 nm) bands, a Multi-Object-Slit medium resolution spectroscopy in a narrow FoV in UV and a simultaneous slitless spectroscopic capability in UV and u bands. To achieve these requirements, several optical design configurations were explored. Here, we present an optical design trade study conducted on various optical design configurations to achieve a sensitivity limit of \(m_{\textrm{AB}}> 26\) mag, in the UV band and a spatial resolution better than 0.2\(^{\prime \prime }\), using a 1-m size telescope aperture. We also present results from our fabrication and alignment tolerance analysis of the selected optical designs, and the design performance that meets the design requirements. Critical parameters like the encircled energy concentration, point spread function (its stability over the field), effects of the spiders supporting the secondary, etc., are explored during the design phase. Based on the trade study conducted in reference to various performance matrices, we down-selected the most optimal optical design for the INSIST.

Abstract Image

印度光谱和成像空间望远镜(坚持):光学设计权衡研究
光学和近红外(NIR)波长的大型地面和天基巡天将在未来十年彻底改变天文学。不幸的是,没有计划中的紫外线(UV)设施来补充这些调查,这对于研究宇宙最活跃的阶段至关重要,包括星系中的恒星形成,活动星系核(AGN),星系团等。一个专门的紫外线任务,印度光谱和成像空间望远镜(坚持),被提议观察紫外线天空。这些引人注目的科学目标确定了一系列高水平的任务要求。根据该计划,该望远镜将具有与印度紫外成像望远镜(UVIT)相当的宽视场(\(\textrm{FoV} \approx 0.25\)平方度),比哈勃太空望远镜大约两个数量级,同时在UV (150-300 nm)、u (300-400 nm)和g (400-550 nm)波段进行视场成像,在紫外窄视场中具有多目标狭缝中分辨率光谱,同时在UV和u波段具有无狭缝光谱能力。为了达到这些要求,我们探索了几种光学设计配置。在这里,我们提出了一项光学设计贸易研究,在不同的光学设计配置下,使用1米口径的望远镜,在紫外波段实现了\(m_{\textrm{AB}}> 26\)等的灵敏度极限和优于0.2 \(^{\prime \prime }\)的空间分辨率。我们还介绍了所选光学设计的制造和对准公差分析结果,以及满足设计要求的设计性能。关键参数,如包围能量集中,点扩散函数(其在场上的稳定性),蜘蛛支撑次要的影响等,在设计阶段进行了探索。在参考各种性能矩阵进行贸易研究的基础上,我们为坚持选择了最优的光学设计。
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来源期刊
Journal of Astrophysics and Astronomy
Journal of Astrophysics and Astronomy 地学天文-天文与天体物理
CiteScore
1.80
自引率
9.10%
发文量
84
审稿时长
>12 weeks
期刊介绍: The journal publishes original research papers on all aspects of astrophysics and astronomy, including instrumentation, laboratory astrophysics, and cosmology. Critical reviews of topical fields are also published. Articles submitted as letters will be considered.
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