In-orbit performance of UVIT over the past 5 years

被引:7
|
作者
Ghosh, S. K. [1 ]
Joseph, P. [2 ]
Kumar, A. [2 ]
Postma, J. [3 ]
Stalin, C. S. [2 ]
Subramaniam, A. [2 ]
Tandon, S. N. [2 ,4 ]
Barve, I., V [2 ]
Devaraj, A. [2 ]
George, K. [2 ,5 ]
Girish, V [6 ]
Hutchings, J. B. [7 ]
Kamath, P. U. [2 ]
Kathiravan, S. [2 ]
Lancelot, J. P. [2 ]
Leahy, D. [3 ]
Mahesh, P. K. [2 ]
Mohan, R. [2 ]
Nagabhushana, S. [2 ]
Pati, A. K. [2 ]
Rao, N. Kameswara [2 ]
Sankarasubramanian, K. [8 ]
Sreekumar, P. [2 ,6 ]
Sriram, S. [2 ]
机构
[1] Tata Inst Fundamental Res, Mumbai 400005, Maharashtra, India
[2] Indian Inst Astrophys, Bangalore 560034, Karnataka, India
[3] Univ Calgary, Calgary, AB, Canada
[4] Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India
[5] Ludwig Maximilian Univ Munich, Munich, Germany
[6] ISRO Headquarters, Bengaluru 560094, India
[7] Natl Res Council Canada, Herzberg Astron & Astrophys, Victoria, BC, Canada
[8] UR Rao Satellite Ctr, Bengaluru 560017, India
关键词
Space vehicles: AstroSat; telescopes: UVIT; instrumentation: astronomical imaging; ULTRAVIOLET IMAGING TELESCOPE;
D O I
10.1007/s12036-020-09685-0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Over the last 5 years, UVIT has completed observations of more than 500 proposals with similar to 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.
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页数:12
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