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Publication Status: Published
Publication Type: Conference contribution, Conference Contribution
Publication year: 2016
Publisher: SPIE
Book Volume: 9905
Article Number: 990515
ISBN: 9781510601895
DOI: 10.1117/12.2233046
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.
APA:
Soffitta, P., Bellazzini, R., Bozzo, E., Burwitz, V., Castro-Tirado, A.J., Costa, E.,... Zoghbi, A. (2016). XIPE: The X-ray imaging polarimetry explorer. In Proceedings of the Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray. SPIE.
MLA:
Soffitta, P., et al. "XIPE: The X-ray imaging polarimetry explorer." Proceedings of the Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray SPIE, 2016.
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