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- Publisher Website: 10.1117/12.3020418
- Scopus: eid_2-s2.0-85207648976
- WOS: WOS:001338129600068
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Conference Paper: The Imaging X-ray Polarimetry Explorer 2.5 years later
Title | The Imaging X-ray Polarimetry Explorer 2.5 years later |
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Authors | |
Keywords | Astrophysics Imaging X-ray Polarimetry Explorer Optics Polarimeters X-ray |
Issue Date | 21-Aug-2024 |
Publisher | SPIE |
Abstract | We have, at last, an observatory dedicated to X-ray polarimetry that has been operational since December 9, 2021. The Imaging X-ray Polarimetry Explorer (IXPE) is a NASA SMEX mission, in partnership with ASI, based on three X-ray telescopes, each equipped with a polarization-sensitive detector in the focus. An extending boom was deployed in orbit, positioning the detectors at the optimal distance from the optics, which have a 4-meter focal length. The spacecraft is three-axis stabilized, providing power, attitude determination and control, transmission, and commanding capabilities. After two and a half years of observation, IXPE has detected positive polarization from nearly all classes of celestial sources that emit X-rays. In this report, we describe the IXPE mission, detailing the performance of the scientific instrumentation after 2.5 years of operation. We also present the main astrophysical results and a few examples of scientific performance during flight. |
Persistent Identifier | http://hdl.handle.net/10722/354660 |
ISBN | |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Ng, Stephen Chi Yung | - |
dc.date.accessioned | 2025-03-02T00:35:12Z | - |
dc.date.available | 2025-03-02T00:35:12Z | - |
dc.date.issued | 2024-08-21 | - |
dc.identifier.isbn | 978-1-5106-7509-4 | - |
dc.identifier.uri | http://hdl.handle.net/10722/354660 | - |
dc.description.abstract | <p>We have, at last, an observatory dedicated to X-ray polarimetry that has been operational since December 9<sup/>, 2021. The Imaging X-ray Polarimetry Explorer (IXPE) is a NASA SMEX mission, in partnership with ASI, based on three X-ray telescopes, each equipped with a polarization-sensitive detector in the focus. An extending boom was deployed in orbit, positioning the detectors at the optimal distance from the optics, which have a 4-meter focal length. The spacecraft is three-axis stabilized, providing power, attitude determination and control, transmission, and commanding capabilities. After two and a half years of observation, IXPE has detected positive polarization from nearly all classes of celestial sources that emit X-rays. In this report, we describe the IXPE mission, detailing the performance of the scientific instrumentation after 2.5 years of operation. We also present the main astrophysical results and a few examples of scientific performance during flight.</p> | - |
dc.language | eng | - |
dc.publisher | SPIE | - |
dc.relation.ispartof | Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray | - |
dc.subject | Astrophysics | - |
dc.subject | Imaging X-ray Polarimetry Explorer | - |
dc.subject | Optics | - |
dc.subject | Polarimeters | - |
dc.subject | X-ray | - |
dc.title | The Imaging X-ray Polarimetry Explorer 2.5 years later | - |
dc.type | Conference_Paper | - |
dc.identifier.doi | 10.1117/12.3020418 | - |
dc.identifier.scopus | eid_2-s2.0-85207648976 | - |
dc.identifier.volume | 13093 | - |
dc.identifier.spage | 1 | - |
dc.identifier.epage | 26 | - |
dc.identifier.isi | WOS:001338129600068 | - |