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Search for Polarization from the Prompt Gamma‐Ray Emission of GRB 041219a with SPI on INTEGRAL

  • Authors: E. Kalemci, S. E. Boggs, C. Kouveliotou, M. Finger, and M. G. Baring

Kalemci et al. 2007 The Astrophysical Journal Supplement Series 169 75.

  • Provider: AAS Journals

Caption: Fig. 6.

Simulated azimuthal scattering angle distribution of 100% polarized photons at 200 keV originating at the GRB position. The center‐to‐center pixellated distribution (black fit) has lower modulation amplitude than the distribution obtained using interaction positions within the detectors (red fit).

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