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小紫外相机(LUVCam1)首次技术演示任务报告

A report on the First Technology Demonstration mission of the Little UV Camera (LUVCam1)

Coby Silayan, Suresh Sivanandam, Aaron Tohuvavohu, Albert Lau, Marianna Dafčíková, Mark Barnet, Patrick Nkwari, Shaojie Chen, Gavin Hay, J. C. Fronteddu, Norbert Werner, Andras Pal, Filip Münz, Jakub Řípa, Emily Hu, Andy Gong

arXiv 2609.21252首次发表:更新:

发表机构

Dunlap Institute for Astronomy & Astrophysics, University of Toronto; David A. Dunlap Department of Astronomy & Astrophysics, University of Toronto; Cosmic Frontier Labs, Oakland, USA; Department of Theoretical Physics and Astrophysics, Faculty of Science, Masaryk University; University of Toronto Institute for Aerospace Studies; Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Budapest, Hungary(多伦多大学邓普天文学与天体物理研究所; 多伦多大学大卫·A·邓普普天文学与天体物理学系; 美国奥克兰宇宙前沿实验室; 马萨里克大学理学院理论与天体物理学系; 多伦多大学航空航天研究学院; 匈牙利布达佩斯地球科学研究中心孔科利天文台)

机构由 AI 辅助整理,请以论文原文为准。

AI 中文总结

本文报告LUVCam1在轨演示结果,验证GSENSE4040 CMOS传感器性能,为QUVIK卫星做准备,并展示利用新航天方法鉴定COTS传感器用于天文任务的可行性。

AI 中文摘要

本文报告了小紫外相机(LUVCam1)首次在轨技术演示的状态。LUVCam1是2024年7月发射的2U立方星GRBBeta上的一个0.4U有效载荷。该任务的主要目标是对GSENSE4040 CMOS传感器及其读出电子学进行鉴定,为快速紫外千新星巡天者(QUVIK;Werner等人,引用\cite{Werner22, Werner24})卫星做准备。LUVCam将作为该任务的主要科学相机。我们报告了LUVCam1上使用的GSENSE4040FSI传感器的性能,首先介绍其实验室表征,然后利用LUVCam1进行的天文观测评估其在轨性能。该相机两年后仍可运行,并拍摄了月球和恒星的图像,我们在此展示。通过LUVCam1,我们展示了一种利用新航天(new-space)方法鉴定最新商用现货(COTS)CMOS传感器用于天文任务的方法。

英文摘要

Here we report on the status of the first on-orbit technology demonstration of the Little UV Camera (LUVCam1). LUVCam1 is a 0.4U payload aboard the 2U cubesat GRBBeta that was launched in July 2024. The primary objective of the mission was to qualify the GSENSE4040 CMOS sensor and its readout electronics in preparation for the Quick UltraVIolet Kilonova Surveyor (QUVIK; Werner et al. \cite{Werner22, Werner24}) satellite. LUVCam will serve as the primary scientific camera for this mission. We report on the performance of the GSENSE4040FSI sensor used on LUVCam1, beginning with its in-lab characterization followed by an assessment of its on-orbit performance using astronomical observations made by LUVCam1. The camera remains operational two years later and has taken pictures of the Moon and stars that we show here. Through LUVCam1, we demonstrated an approach leveraging new-space to qualify the latest COTS CMOS sensors for astronomy missions.

Comments19 pages, 18 figures; SPIE Astronomical Telescopes + Instrumentation Conference Proceedings

DOI:10.1117/12.3104899

论文原文

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