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After two and a half years of observation, IXPE has detected positive polarization from nearly all classes of celestial sources that emit X-rays. In this report, we describe the IXPE mission, detailing the performance of the scientific instrumentation after 2.5 years of operation. We also present the main astrophysical results and a few examples of scientific performance during flight.
Next activities are oriented to realize a Digital Pulse Processor readout electronics implemented in such a way that, in the future, it can be built with space-qualified components. The system shall be able to manage flux variations of several orders of magnitude to deal with the extreme Sun conditions: from quiet to the most energetic class-X flares. Beside this, an activity to identify which are the possible signatures of solar events is on-going.
This paper reports the current and the planned activities to implement the sensor’s readout functions in an FPGA-based space-ready electronics.
The LAD instrument has now completed the assessment phase but was not down-selected for launch. However, during the assessment, most of the trade-offs have been closed leading to a robust and well documented design that will be reproposed in future ESA calls. In this talk, we will summarize the characteristics of the LAD design and give an overview of the expectations for the instrument capabilities.
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