XIPE: The X-ray imaging polarimetry explorer

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 d...

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Detalles Bibliográficos
Publicado:	2016
Materias:	Gas Pixel Detector Polarimetry X-ray Astronomy X-ray optics Astrophysics Ellipsometry Photoelectricity Pixels Polarimeters Readout systems Space telescopes X ray analysis X ray optics Effective area Fundamental physics Large effective areas Pixel detector Spatially resolved United kingdom X-ray astronomy X-ray polarimetry Gamma rays
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0277786X_v9905_n_p_Soffitta http://hdl.handle.net/20.500.12110/paper_0277786X_v9905_n_p_Soffitta
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

id	paper:paper_0277786X_v9905_n_p_Soffitta
record_format	dspace
spelling	paper:paper_0277786X_v9905_n_p_Soffitta2023-06-08T15:26:39Z XIPE: The X-ray imaging polarimetry explorer Gas Pixel Detector Polarimetry X-ray Astronomy X-ray optics Astrophysics Ellipsometry Photoelectricity Pixels Polarimeters Readout systems Space telescopes X ray analysis X ray optics Effective area Fundamental physics Large effective areas Pixel detector Spatially resolved United kingdom X-ray astronomy X-ray polarimetry Gamma rays 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. © 2016 SPIE. 2016 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0277786X_v9905_n_p_Soffitta http://hdl.handle.net/20.500.12110/paper_0277786X_v9905_n_p_Soffitta
institution	Universidad de Buenos Aires
institution_str	I-28
repository_str	R-134
collection	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic	Gas Pixel Detector Polarimetry X-ray Astronomy X-ray optics Astrophysics Ellipsometry Photoelectricity Pixels Polarimeters Readout systems Space telescopes X ray analysis X ray optics Effective area Fundamental physics Large effective areas Pixel detector Spatially resolved United kingdom X-ray astronomy X-ray polarimetry Gamma rays
spellingShingle	Gas Pixel Detector Polarimetry X-ray Astronomy X-ray optics Astrophysics Ellipsometry Photoelectricity Pixels Polarimeters Readout systems Space telescopes X ray analysis X ray optics Effective area Fundamental physics Large effective areas Pixel detector Spatially resolved United kingdom X-ray astronomy X-ray polarimetry Gamma rays XIPE: The X-ray imaging polarimetry explorer
topic_facet	Gas Pixel Detector Polarimetry X-ray Astronomy X-ray optics Astrophysics Ellipsometry Photoelectricity Pixels Polarimeters Readout systems Space telescopes X ray analysis X ray optics Effective area Fundamental physics Large effective areas Pixel detector Spatially resolved United kingdom X-ray astronomy X-ray polarimetry Gamma rays
description	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. © 2016 SPIE.
title	XIPE: The X-ray imaging polarimetry explorer
title_short	XIPE: The X-ray imaging polarimetry explorer
title_full	XIPE: The X-ray imaging polarimetry explorer
title_fullStr	XIPE: The X-ray imaging polarimetry explorer
title_full_unstemmed	XIPE: The X-ray imaging polarimetry explorer
title_sort	xipe: the x-ray imaging polarimetry explorer
publishDate	2016
url	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0277786X_v9905_n_p_Soffitta http://hdl.handle.net/20.500.12110/paper_0277786X_v9905_n_p_Soffitta
_version_	1768545645845544960

XIPE: The X-ray imaging polarimetry explorer

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