Authors

Michela Negro, University of Maryland, Baltimore County (UMBC)
Niccolò Di Lalla, Kavli Institute for Particle Astrophysics and Cosmology
Nicola Omodei, Kavli Institute for Particle Astrophysics and Cosmology
Péter Veres, Department of Space Science
Stefano Silvestri, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Alberto Manfreda, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Eric Burns, Louisiana State University
Luca Baldini, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Enrico Costa, Istituto Nazionale Di Astrofisica, Rome
Steven R. Ehlert, NASA Marshall Space Flight Center
Jamie A. Kennea, Pennsylvania State University
Ioannis Liodakis, Turun yliopisto
Herman L. Marshall, MIT Kavli Institute for Astrophysics and Space Research
Sandro Mereghetti, INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
Riccardo Middei, Agenzia Spaziale Italiana
Fabio Muleri, Istituto Nazionale Di Astrofisica, Rome
Stephen L. O’Dell, NASA Marshall Space Flight Center
Oliver J. Roberts, Huntsville Program Office
Roger W. Romani, Kavli Institute for Particle Astrophysics and Cosmology
Carmelo Sgró, Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
Masanobu Terashima, Yamagata University
Andrea Tiengo, INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
Domenico Viscolo, Università di Pisa
Alessandro Di Marco, Istituto Nazionale Di Astrofisica, Rome
Fabio La Monaca, Istituto Nazionale Di Astrofisica, Rome
Luca Latronico, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
Giorgio Matt, Università degli Studi Roma Tre
Matteo Perri, Agenzia Spaziale Italiana
Simonetta Puccetti, Agenzia Spaziale Italiana
Juri Poutanen, Turun yliopisto
Ajay Ratheesh, Istituto Nazionale Di Astrofisica, Rome
Daniele Rogantini, MIT Kavli Institute for Astrophysics and Space Research
Patrick Slane, Harvard-Smithsonian Center for Astrophysics

Document Type

Article

Publication Date

3-1-2023

Abstract

We present the IXPE observation of GRB 221009A, which includes upper limits on the linear polarization degree of both prompt and afterglow emission in the soft X-ray energy band. GRB 221009A is an exceptionally bright gamma-ray burst (GRB) that reached Earth on 2022 October 9 after traveling through the dust of the Milky Way. The Imaging X-ray Polarimetry Explorer (IXPE) pointed at GRB 221009A on October 11 to observe, for the first time, the 2-8 keV X-ray polarization of a GRB afterglow. We set an upper limit to the polarization degree of the afterglow emission of 13.8% at a 99% confidence level. This result provides constraints on the jet opening angle and the viewing angle of the GRB, or alternatively, other properties of the emission region. Additionally, IXPE captured halo-rings of dust-scattered photons that are echoes of the GRB prompt emission. The 99% confidence level upper limit to the prompt polarization degree depends on the background model assumption, and it ranges between ∼55% and ∼82%. This single IXPE pointing provides both the first assessment of X-ray polarization of a GRB afterglow and the first GRB study with polarization observations of both the prompt and afterglow phases.

Publication Source (Journal or Book title)

Astrophysical Journal Letters

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