XIPE: The X-ray imaging polarimetry explorer
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A4 Artikkeli konferenssijulkaisussa
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Date
2016
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Language
en
Pages
20
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Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, Volume 9905, Proceedings of SPIE : the International Society for Optical Engineering, issue 9905
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.Description
Keywords
Gas Pixel Detector, Polarimetry, X-ray Astronomy, X-ray optics
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L, Zdziarski, A A, Zech, A, Zhang, H, Zhang, S, Zhang, S, Zhang, W & Zoghbi, A 2016, XIPE : The X-ray imaging polarimetry explorer . in J-W A den Herder, T Takahashi & M Bautz (eds), Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray . vol. 9905, 990515, Proceedings of SPIE : the International Society for Optical Engineering, no. 9905, SPIE, Space Telescopes and Instrumentation, Edinburgh, United Kingdom, 26/06/2016 . https://doi.org/10.1117/12.2233046