DOI | Resolve DOI: https://doi.org/10.1117/12.2056518 |
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Author | Search for: Hutchings, J. B.1 |
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Affiliation | - National Research Council of Canada. National Science Infrastructure
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Format | Text, Article |
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Conference | Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, June 22-26, 2014 |
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Subject | image reconstruction; imaging techniques; observatories; space telescopes; multi-wavelengths; resolution imaging; space; ultraviolet; visible band; X-ray telescope; Gamma rays |
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Abstract | UVIT consists of two co-aligned 38cm telescopes that provide ∼1 arsec resolution imaging over 28 arcmin fields, in FUV, NUV, and Visible bands simultaneously. Each channel has a choice of filters, and, for the UV channels, gratings. UVIT is also co-aligned with three X-ray telescopes on the observatory, and all operate together. This paper gives details of the operation and performance of the instrument. |
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Publication date | 2014-07-24 |
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Publisher | SPIE |
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In | |
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Series | |
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Language | English |
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Peer reviewed | Yes |
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NPARC number | 21275460 |
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Export citation | Export as RIS |
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Report a correction | Report a correction (opens in a new tab) |
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Record identifier | f36c0de1-e32f-4aeb-915c-31ad435db2e7 |
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Record created | 2015-07-14 |
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Record modified | 2020-04-22 |
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