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The Calibration of the UVIT Detectors for the ASTROSAT Observatory

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dc.contributor.author Leahy, Denis
dc.contributor.author Postma, J
dc.contributor.author Hutchings, J. B
dc.contributor.author Tandon, S. N
dc.date.accessioned 2020-11-27T12:49:40Z
dc.date.available 2020-11-27T12:49:40Z
dc.date.issued 2018-08
dc.identifier.citation Proceedings of the International Astronomical Union, Vol. 30, pp. 487-491 en_US
dc.identifier.issn 1743-9213
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7486
dc.description Restricted Access © International Astronomical Union https://doi.org/10.1017/S1743921319005180 en_US
dc.description.abstract The UVIT ultraviolet and visual band detectors and electronics for the ASTROSAT observatory were calibrated in the vacuum laboratory at the University of Calgary. This work was supported by the Canadian Space Agengy and carried out prior to integration with the UVIT optical assembly and the ASTROSAT spacecraft. The multiband (X-ray, ultraviolet and optical) ASTROSAT observatory was successfully launched by the Indian Space Research Organization on Sept. 28, 2015, with subsequent in-orbit verification and ongoing calibration activities. Here we discuss the current issues of calibrating the UVIT data, such as distortion corrections, and how the laboratory data is being used to address these issues. en_US
dc.language.iso en en_US
dc.publisher Cambridge University Press en_US
dc.relation.ispartofseries IAU Focus Meetings No. 30;
dc.subject instrumentation: detectors en_US
dc.subject techniques: image processing en_US
dc.subject techniques: photometric en_US
dc.title The Calibration of the UVIT Detectors for the ASTROSAT Observatory en_US
dc.type Article en_US


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