| DOI | Resolve DOI: https://doi.org/10.3847/1538-3881/aa8451 |
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| Author | Search for: Tandon, S. N.; Search for: Subramaniam, Annapurni; Search for: Girish, V.; Search for: Postma, J.; Search for: Sankarasubramanian, K.; Search for: Sriram, S.; Search for: Stalin, C. S.; Search for: Mondal, C.; Search for: Sahu, S.; Search for: Joseph, P.; Search for: Hutchings, J.1; Search for: Ghosh, S. K.; Search for: Barve, I. V.; Search for: George, K.; Search for: Kamath, P. U.; Search for: Kathiravan, S.; Search for: Kumar, A.; Search for: Lancelot, J. P.; Search for: Leahy, D.; Search for: Mahesh, P. K.; Search for: Mohan, R.; Search for: Nagabhushana, S.; Search for: Pati, A. K.; Search for: Kameswara rao, N.; Search for: Sreedhar, Y. H.; Search for: Sreekumar, P. |
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| Affiliation | - National Research Council of Canada. Herzberg Astronomy and Astrophysics
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| Format | Text, Article |
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| Abstract | The Ultra-Violet Imaging Telescope (UVIT) is one of the payloads in ASTROSAT, the first Indian Space Observatory. The UVIT instrument has two 375 mm telescopes: one for the far-ultraviolet (FUV) channel (1300–1800 Å), and the other for the near-ultraviolet (NUV) channel (2000–3000 Å) and the visible (VIS) channel (3200–5500 Å). UVIT is primarily designed for simultaneous imaging in the two ultraviolet channels with spatial resolution better than 1farcs8, along with provisions for slit-less spectroscopy in the NUV and FUV channels. The results of in-orbit calibrations of UVIT are presented in this paper. |
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| Publication date | 2017-09-01 |
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| Publisher | IOP |
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| In | |
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| Language | English |
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| Peer reviewed | Yes |
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| NPARC number | 23003115 |
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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 | 36408c55-59b6-4e2a-82fa-dd72cc6d99b2 |
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| Record created | 2018-04-20 |
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| Record modified | 2020-03-16 |
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