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X-Ray Polarization of the Magnetar 1E 1841−045

  • Authors: Rachael Stewart, George A. Younes, Alice K. Harding, Zorawar Wadiasingh, Matthew G. Baring, Michela Negro, Tod E. Strohmayer, Wynn C. G. Ho, Mason Ng, Zaven Arzoumanian, Hoa Dinh Thi, Niccolò Di Lalla, Teruaki Enoto, Keith Gendreau, Chin-Ping Hu, Alex van Kooten, Chryssa Kouveliotou, Alexander McEwen

Rachael Stewart et al 2025 The Astrophysical Journal Letters 985 .

  • Provider: AAS Journals

Caption: Figure 3.

Phase-resolved polarization characteristics of 1E 1841−045. The columns display the intensity pulse profiles (top row), polarization degree (center), and polarization angle (bottom row) according to 2–4 keV (left column), 4–8 keV (central column), and 2–8 keV (right column). The phasograms are divided according to five phase bins (shown in colored vertical bands) that correspond to morphological features of the IXPE energy-integrated intensity pulse profile. The corresponding MDP99 for each phase and energy bin are shown as overlapping shaded regions.

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