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Opto-mechanical assembly and ground calibration of LUCI

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dc.contributor.author Mathew, J
dc.contributor.author Nair, B. G
dc.contributor.author Sriram, S
dc.contributor.author Kamath, P. U
dc.contributor.author Prakash, A
dc.contributor.author Mayuresh, Sarpotdar
dc.contributor.author Ambily, S
dc.contributor.author Nirmal, K
dc.contributor.author Sreejith, A. G
dc.contributor.author Safonova, M
dc.contributor.author Murthy, J
dc.contributor.author Brosch, N
dc.date.accessioned 2020-11-12T15:02:29Z
dc.date.available 2020-11-12T15:02:29Z
dc.date.issued 2018-08-20
dc.identifier.citation Proceedings of the SPIE, Vol. 10699, pp.106992V-1-106992V-10 en_US
dc.identifier.issn 1996-756X
dc.identifier.uri http://prints.iiap.res.in/handle/2248/6947
dc.description Restricted Access © SPIE--The International Society for Optical Engineering https://doi.org/10.1117/12.2312733 en_US
dc.description.abstract The Lunar Ultraviolet Cosmic Imager (LUCI) is an innovative all-spherical mirrors telescope, proposed to fly as a scientific UV imaging payload on a lunar mission in collaboration with Indian Aerospace Company-TeamIndus, Axiom Research Labs Pvt. Ltd. Observations from the Moon provide a unique opportunity to observe the sky from a stable platform far above the Earths atmosphere. LUCI will observe at a fixed elevation angle and will detect stars in the near ultraviolet (200-320 nm) to a limiting magnitude of 12 AB, with a field of view of around 0.5 degrees. The primary science goal is to search for transient sources and flag them for further study. The instrument has been assembled in the class 1000 clean room at the M.G.K Menon Laboratory for Space Sciences. Here we will describe the optomechanical assembly procedures we have carried out during the optical alignment and integration of the payload. Opto-mechanical alignment of the instrument was carried out by using alignment telescope cum autocollimator (for coarse alignment) and ZYGO interferometer (fine alignment). We will also discuss the ground calibration tests performed on the assembled telescope. The results from the ground calibration activities will help in establishing the full calibration matrix of the instrument once operational. en_US
dc.language.iso en en_US
dc.publisher SPIE--The International Society for Optical Engineering en_US
dc.subject UV space instrumentation en_US
dc.subject Opto-mechanical assembly en_US
dc.subject Calibration en_US
dc.subject UV astronomy en_US
dc.title Opto-mechanical assembly and ground calibration of LUCI en_US
dc.type Article en_US


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