Soft X-ray Focusing Telescope Aboard AstroSat: Design, Characteristics and Performance
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The Soft X-ray focusing Telescope (SXT), India’s first X-ray telescope based on the principle of grazing incidence, was launched aboard the AstroSat and made operational on October 26, 2015. X-rays in the energy band of 0.3–8.0 keV are focussed on to a cooled charge coupled device thus providing medium resolution X-ray spectroscopy of cosmic X-ray sources of various types. It is the most sensitive X-ray instrument aboard the AstroSat. In its first year of operation, SXT has been used to observe objects ranging from active stars, compact binaries, supernova remnants, active galactic nuclei and clusters of galaxies in order to study its performance and quantify its characteriztics. Here, we present an overview of its design, mechanical hardware, electronics, data modes, observational constraints, pipeline processing and its in-orbit performance based on preliminary results from its characterization during the performance verification phase.
KeywordsSpace vehicles: instruments instrumentation: detectors.
The Tata Institute of Fundamental Research (TIFR), Mumbai, led the effort with instrument design, development, integration and testing of the SXT. The Space Research Centre of the University of Leicester, UK, led the development of the Focal Plane Camera for which the processing electronics was built at TIFR. Vikram Sarabhai Space Centre, Thiruvananthapuram provided the CFRP tubular structures for the SXT. The door mechanism for the telescope, the radiator plate and the heat pipe were developed at the ISRO Satellite Centre, Bengaluru. The Space Application Centre (SAC), Ahmedabad, TIFR, Mumbai and IUCAA, Pune jointly developed the analysis software. A vast number of industries participated in the fabrication of infrastructure and mechanical components of the SXT. ISRO funded, managed and facilitated the project. Various softwares including Python, IDL, FTOOLS, C and C++ were also used.
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