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Ultraviolet Imaging Telescope on AstroSat

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dc.contributor.author Tandon, S. N
dc.contributor.author Ghosh, S. K
dc.contributor.author Hutchings, J
dc.contributor.author Stalin, C. S
dc.contributor.author Subramaniam, A
dc.date.accessioned 2020-11-10T02:32:31Z
dc.date.available 2020-11-10T02:32:31Z
dc.date.issued 2017-08
dc.identifier.citation Current Science, Vol. 113, No. 4, pp. 583 - 586 en_US
dc.identifier.issn 0011-3891
dc.identifier.uri http://prints.iiap.res.in/handle/2248/6735
dc.description Open Access © Current Science Association http://www.currentscience.ac.in/Volumes/113/04/0583.pdf en_US
dc.description.abstract The AstroSat satellite is designed for multiwavelength astronomy for observations covering a spectral range from soft and hard X-rays to the ultraviolet. The Ultraviolet Imaging Telescope (UVIT) is the only non-X-ray telescope on AstroSat and it provides the long lever arm to the multi-wavelength observations. In addition to the simultaneous multiwavelength studies in coordination with the X-ray telescopes on-board AstroSat, UVIT is used to study a large variety of objects with arcsecond-level spatial resolution. During the first year of observations, UVIT has obtained images in many filter bands in the wavelength range 130–300 nm over a field of ~28, which are being used to study a variety of hot stars, nebulae, stellar clusters and galaxies. en_US
dc.language.iso en en_US
dc.publisher Current Science Association en_US
dc.subject Multi-wavelength astronomy en_US
dc.subject Ultraviolet Imaging Telescope en_US
dc.subject X-ray telescope en_US
dc.title Ultraviolet Imaging Telescope on AstroSat en_US
dc.type Article en_US


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