XIPE: the x-ray imaging polarimetry explorer
| Authors |
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| Publication date | 2016 |
| Host editors |
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| Book title | Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray |
| Book subtitle | 26 June-1 July 2016, Edinburgh, United Kingdom |
| ISBN |
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| ISBN (electronic) |
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| 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 |
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| 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.
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| 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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