Share Email Print
cover

Proceedings Paper

The DRE: the digital readout electronics for ATHENA X-IFU
Author(s): Laurent Ravera; Christophe Cara; María Teresa Ceballos; Xavier Barcons; Didier Barret; Rodolphe Clédassou; Antoine Clénet; Beatriz Cobo; Eric Doumayrou; Roland H. den Hartog; Bert-Joost van Leeuwen; Dennis van Loon; José Miguel Mas-Hesse; Claude Pigot; Etienne Pointecouteau
Format Member Price Non-Member Price
PDF $14.40 $18.00

Paper Abstract

We are developing the digital readout electronics (DRE) of the X-Ray Integral Field Unit (X-IFU), one of the two Athena focal plane instruments. This subsystem is made of two main parts: the DRE-DEMUX and the DRE-EP. With a frequency domain multiplexing (FDM) the DRE-DEMUX makes the readout of the 3 840 Transition Edge Sensors (TES) in 96 channels of 40 pixels each. It provides the AC signals to voltage-bias the TES, it demodulates the detector's data which are readout by a SQUID and low noise amplifiers and it linearizes the detection chain to increase its dynamic range. The feedback is computed with a specific technique, so called baseband feedback (BBFB) which ensures that the loop is stable even with long propagation and processing delays (i.e. a few μs) and with high frequency AC-bias (up to 5 MHz). This processing is partly analogue (anti aliasing and reconstruction filters) but mostly digital. The digital firmware is simultaneously applied to all the pixels in digital integrated circuits. After the demultiplexing the interface between the DRE-DEMUX and the DRE-EP has to cope with a data rate of 61.44 Gbps to transmit the data of the individual pixels. Then, the DRE-EP detects the events and computes their energy and grade according to their spectral quality: low resolution, medium resolution and high resolution (i.e. if two consecutive events are too close the estimate of the energy is less accurate). This processing is done in LEON based processor boards. At its output the DRE-EP provides the control unit of the instrument with a list including for each event its time of arrival, its energy, its location on the focal plane and its grade.

Paper Details

Date Published: 24 July 2014
PDF: 8 pages
Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91445T (24 July 2014); doi: 10.1117/12.2055750
Show Author Affiliations
Laurent Ravera, Observatoire Midi-Pyrénées, IRAP, CNRS, Univ. de Toulouse (France)
Christophe Cara, CEA Saclay (France)
María Teresa Ceballos, Instituto de Física de Cantabria, CSIC, Univ. de Cantabria (Spain)
Xavier Barcons, Instituto de Física de Cantabria, CSIC, Univ. de Cantabria (Spain)
Didier Barret, Observatoire Midi-Pyrénées, IRAP, CNRS, Univ. de Toulouse (France)
Rodolphe Clédassou, Ctr. National d'Études Spatiales (France)
Antoine Clénet, Observatoire Midi-Pyrénées, IRAP, CNRS, Univ. de Toulouse (France)
Beatriz Cobo, Instituto de Física de Cantabria, CSIC, Univ. de Cantabria (Spain)
Eric Doumayrou, CEA Saclay (France)
Roland H. den Hartog, SRON Netherlands Institute for Space Research (Netherlands)
Bert-Joost van Leeuwen, SRON Netherlands Institute for Space Research (Netherlands)
Dennis van Loon, SRON Netherlands Institute for Space Research (Netherlands)
José Miguel Mas-Hesse, Instituto Nacional de Técnica Aeroespacial, CSIC (Spain)
Claude Pigot, CEA Saclay (France)
Etienne Pointecouteau, Observatoire Midi-Pyrénées, IRAP, CNRS, Univ. de Toulouse (France)


Published in SPIE Proceedings Vol. 9144:
Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
Tadayuki Takahashi; Jan-Willem A. den Herder; Mark Bautz, Editor(s)

© SPIE. Terms of Use
Back to Top