Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6701
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dc.contributor.authorMurthy, J-
dc.contributor.authorRahna, P. T-
dc.contributor.authorSutaria, F. K-
dc.contributor.authorSafonova, M-
dc.contributor.authorGudennavar, S. B-
dc.contributor.authorBubbly, S. G-
dc.date.accessioned2020-11-10T01:59:39Z-
dc.date.available2020-11-10T01:59:39Z-
dc.date.issued2017-07-
dc.identifier.citationAstronomy and Computing, Vol. 20, pp. 120-127en_US
dc.identifier.issn2213-1337-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6701-
dc.descriptionRestricted Access © Elsevier B.V. https://doi.org/10.1016/j.ascom.2017.07.001en_US
dc.description.abstractThe Ultraviolet Imaging Telescope (UVIT) was launched as part of the multi-wavelength Indian AstroSat mission on 28 September, 2015 into a low Earth orbit. A 6-month performance verification (PV) phase ended in March 2016, and the instrument is now in the general observing phase. UVIT operates in three channels: visible, near-ultraviolet (NUV) and far-ultraviolet (FUV), each with a choice of broad and narrow band filters, and has NUV and FUV gratings for low-resolution spectroscopy. We have written a software package (JUDE ) to convert the Level 1 data from UVIT into scientifically useful photon lists and images. The routines are written in the GNU Data Language (GDL) and are compatible with the IDL software package. We use these programs in our own scientific work, and will continue to update the programs as we gain better understanding of the UVIT instrument and its performance. We have released JUDE under an Apache License.en_US
dc.language.isoenen_US
dc.publisherElsevier B.Ven_US
dc.subjectUltravioleten_US
dc.subjectUVITen_US
dc.subjectAstronomical softwareen_US
dc.subjectData analysisen_US
dc.titleJUDE: an ultraviolet imaging telescope pipelineâen_US
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