The Imaging X-ray Polarimetry Explorer (IXPE) will add linear polarization (degree and angle) to the usual features (time, energy, and position) typical of an x-ray astronomy mission. It will expand the available information. IXPE is a NASA Astrophysics Small Explorer (SMEX) mission with a large contribution by ASI which will be launched into an equatorial orbit in 2021. While several non-useful upper limits are available back from the'70 the two order of magnitude improvement of IXPE mission will provide meaningful observations among few dozen sources in the 2-8 keV band. Thanks to its imaging capabilities, it will be possible to produce for the first time polarization maps of several X-ray-bright extended sources. Thanks to its sensitivity, also phase-resolved polarimetry of many bright pulsating x-ray sources will be available.

The Imaging X-ray polarimetry explorer (IXPE): Technical overview III

Maldera S.;Orsini L.;Bonino R.;Massaro F.;Paggi A.;
2020-01-01

Abstract

The Imaging X-ray Polarimetry Explorer (IXPE) will add linear polarization (degree and angle) to the usual features (time, energy, and position) typical of an x-ray astronomy mission. It will expand the available information. IXPE is a NASA Astrophysics Small Explorer (SMEX) mission with a large contribution by ASI which will be launched into an equatorial orbit in 2021. While several non-useful upper limits are available back from the'70 the two order of magnitude improvement of IXPE mission will provide meaningful observations among few dozen sources in the 2-8 keV band. Thanks to its imaging capabilities, it will be possible to produce for the first time polarization maps of several X-ray-bright extended sources. Thanks to its sensitivity, also phase-resolved polarimetry of many bright pulsating x-ray sources will be available.
2020
Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
usa
2020
Proceedings of SPIE - The International Society for Optical Engineering
SPIE
11444
245
256
9781510636750
9781510636767
Astrophysics; Gas Pixel Detector; Optics; Polarimetry; X-ray
Soffitta P.; Attina P.; Baldini L.; Barbanera M.; Baumgartner W.H.; Bellazzini R.; Bladt J.; Bongiorno S.D.; Brez A.; Castellano S.; Carpentiero R.; C...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/1872906
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