XIPE: the x-ray imaging polarimetry explorer

Authors
Publication date 2016
Host editors
  • J.-W.A. den Herder
  • T. Takahashi
  • M. Bautz
Book title Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Book subtitle 26 June-1 July 2016, Edinburgh, United Kingdom
ISBN
  • 9781510601895
ISBN (electronic)
  • 9781510601901
Series Proceedings of SPIE
Event Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Article number 990515
Volume | Issue number 1
Number of pages 20
Publisher Bellingham, WA: SPIE
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract
XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror but with a low weight. The payload is compatible with the fairing of the Vega launcher. XIPE is designed as an observatory for X-ray astronomers with 75 % of the time dedicated to a Guest Observer competitive program and it is organized as a consortium across Europe with main contributions from Italy, Germany, Spain, United Kingdom, Poland, Sweden.
Document type Conference contribution
Language English
Published at https://doi.org/10.1117/12.2233046
Other links http://adsabs.harvard.edu/abs/2016SPIE.9905E..15S
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