UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXI 2019
DOI: 10.1117/12.2530646
|View full text |Cite
|
Sign up to set email alerts
|

The Imaging X-Ray Polarimetry Explorer (IXPE): technical overview II

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...

Citation Types

0
1
0

Year Published

2020
2020
2021
2021

Publication Types

Select...
3
2

Relationship

0
5

Authors

Journals

citations
Cited by 8 publications
(1 citation statement)
references
References 6 publications
0
1
0
Order By: Relevance
“…Indeed, a single significant polarimetric measurement exists in the soft X-ray band, dating back to the flight of a Bragg polarimeter on-board OSO-8 more than 40 years ago ( [1]), which measured a linear polarization degree for the Crab Nebula of (19.2 ± 1.0)% at 2.6 keV. Things are expected to change in the near future, thanks to the forthcoming Imaging X-ray Polarimetry Explorer (IXPE) mission [2], which will be entirely dedicated to X-ray polarimetry. Selected in January 2017 by NASA as its next SMEX (SMall EXplorer1) mission IXPE is funded by a partnership between NASA and ASI.2 It is scheduled for launch in mid 2021 and will operate for two years, plus one of possible extension, allowing the polarimetric observation of dozens of celestial objects in the 2-8 keV energy band.…”
mentioning
confidence: 99%
“…Indeed, a single significant polarimetric measurement exists in the soft X-ray band, dating back to the flight of a Bragg polarimeter on-board OSO-8 more than 40 years ago ( [1]), which measured a linear polarization degree for the Crab Nebula of (19.2 ± 1.0)% at 2.6 keV. Things are expected to change in the near future, thanks to the forthcoming Imaging X-ray Polarimetry Explorer (IXPE) mission [2], which will be entirely dedicated to X-ray polarimetry. Selected in January 2017 by NASA as its next SMEX (SMall EXplorer1) mission IXPE is funded by a partnership between NASA and ASI.2 It is scheduled for launch in mid 2021 and will operate for two years, plus one of possible extension, allowing the polarimetric observation of dozens of celestial objects in the 2-8 keV energy band.…”
mentioning
confidence: 99%