Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7486
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dc.contributor.authorLeahy, Denis-
dc.contributor.authorPostma, J-
dc.contributor.authorHutchings, J. B-
dc.contributor.authorTandon, S. N-
dc.date.accessioned2020-11-27T12:49:40Z-
dc.date.available2020-11-27T12:49:40Z-
dc.date.issued2018-08-
dc.identifier.citationProceedings of the International Astronomical Union, Vol. 30, pp. 487-491en_US
dc.identifier.issn1743-9213-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7486-
dc.descriptionRestricted Access © International Astronomical Union https://doi.org/10.1017/S1743921319005180en_US
dc.description.abstractThe 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.isoenen_US
dc.publisherCambridge University Pressen_US
dc.relation.ispartofseriesIAU Focus Meetings No. 30;-
dc.subjectinstrumentation: detectorsen_US
dc.subjecttechniques: image processingen_US
dc.subjecttechniques: photometricen_US
dc.titleThe Calibration of the UVIT Detectors for the ASTROSAT Observatoryen_US
dc.typeArticleen_US
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