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In-orbit performance of UVIT over the past 5 years

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dc.contributor.author Ghosh, S. K
dc.contributor.author Joseph, P
dc.contributor.author Kumar, A
dc.contributor.author Postma, J
dc.contributor.author Stalin, C. S
dc.contributor.author Subramaniam, A
dc.contributor.author Tandon, S. N
dc.contributor.author Barve, Indrajit V
dc.contributor.author Devaraj, A
dc.contributor.author George, K
dc.contributor.author Girish, V
dc.contributor.author Hutchings, J. B
dc.contributor.author Kamath, P. U
dc.contributor.author Kathiravan, S
dc.contributor.author Lancelot, J. P
dc.contributor.author Leahy, D
dc.contributor.author Mahesh, P. K
dc.contributor.author Mohan, R
dc.contributor.author Nagabhushana, S
dc.contributor.author Pati, A. K
dc.contributor.author Kameswara Rao, N
dc.contributor.author Sankarasubramanian, K
dc.contributor.author Sreekumar, P
dc.contributor.author Sriram, S
dc.date.accessioned 2021-07-23T05:36:26Z
dc.date.available 2021-07-23T05:36:26Z
dc.date.issued 2021-10
dc.identifier.citation Journal of Astrophysics and Astronomy, Vol. 42, No. 2, 20 en_US
dc.identifier.issn 0973-7758
dc.identifier.uri http://hdl.handle.net/2248/7812
dc.description Restricted Access en_US
dc.description The original publication is available at springerlink.com
dc.description.abstract Over the last 5 years, UVIT has completed observations of more than 500 proposals with ∼800 unique pointings. In addition, regular planned monitoring observations have been made and from their analysis various key parameters related to in orbit performance of UVIT have been quantified. The sensitivities of the UV channels have remained steady indicating no effect of potential molecular contamination confirming the adequacy of all the protocols implemented for avoiding contamination. The quality of the PSF through the years confirms adequacy of thermal control measures. The early calibrations obtained during the Performance Verification (PV) phase have been further revised for more subtle effects. These include flat fields and detector distortions with greater precision. The operations of UVIT have also evolved through in orbit experience, e.g. tweaking of operational sequencing, protocol for recovery from bright object detection (BOD) shutdowns, parameters for BOD thresholds, etc. Finally, some effects of charged particle hits on electronics led to opimised strategy for regular resetting. The Near-UV channel was lost in one of such operations. All the above in-orbit experiences are presented here. en_US
dc.language.iso en en_US
dc.publisher Indian Academy of Sciences en_US
dc.relation.uri https://doi.org/10.1007/s12036-020-09685-0
dc.rights © Indian Academy of Sciences
dc.subject Space vehicles: AstroSat en_US
dc.subject Telescopes: UVIT en_US
dc.subject Instrumentation: astronomical imaging en_US
dc.title In-orbit performance of UVIT over the past 5 years en_US
dc.type Article en_US


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