Authors

Paolo Soffitta, Istituto Nazionale Di Astrofisica, Rome
Luca Baldini, Università di Pisa
Wayne Baumgartner, NASA Marshall Space Flight Center
Ronaldo Bellazzini, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Stephen D. Bongiorno, NASA Marshall Space Flight Center
Niccolò Bucciantini, Osservatorio Astrofisico Di Arcetri
Enrico Costa, Istituto Nazionale Di Astrofisica, Rome
Michal Dovčiak, Academy of Sciences of the Czech Republic
Steven Ehlert, NASA Marshall Space Flight Center
Philip E. Kaaret, NASA Marshall Space Flight Center
Jeffery J. Kolodziejczak, NASA Marshall Space Flight Center
Luca Latronico, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
Frédréic Marin, Observatoire Astronomique de Strasbourg
Alan P. Marscher, Boston University
Herman L. Marshall, MIT Kavli Institute for Astrophysics and Space Research
Giorgio Matt, Università degli Studi Roma Tre
Fabio Muleri, Istituto Nazionale Di Astrofisica, Rome
Stephen L. O'Dell, NASA Marshall Space Flight Center
Juri Poutanen, Turun yliopisto
Brian Ramsey, NASA Marshall Space Flight Center
Roger W. Romani, Kavli Institute for Particle Astrophysics and Cosmology
Patrick Slane, Harvard-Smithsonian Center for Astrophysics
Allyn F. Tennant, NASA Marshall Space Flight Center
Roberto Turolla, Università degli Studi di Padova
Martin C. Weisskopf, NASA Marshall Space Flight Center
Iván Agudo, CSIC - Instituto de Astrofísica de Andalucía (IAA)
Lucio Angelo Antonelli, Osservatorio Astronomico di Roma
Matteo Bachetti, Osservatorio Astronomico di Cagliari
Stefano Bianchi, Università degli Studi Roma Tre
Raffaella Bonino, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
Alessandro Brez, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Fiamma Capitanio, Istituto Nazionale Di Astrofisica, Rome
Simone Castellano, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa

Document Type

Conference Proceeding

Publication Date

1-1-2024

Abstract

We have, at last, an observatory dedicated to X-ray polarimetry that has been operational since December 9th, 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.

Publication Source (Journal or Book title)

Proceedings of SPIE the International Society for Optical Engineering

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