Fig. 8 from Search for Polarization from the Prompt Gamma‐Ray Emission of GRB 041219a with SPI on INTEGRAL

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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. 8.

Simulated modulation factors for GRB 041219a (100–350 keV) as a function of polarization angle. Interaction positions within detectors are used to obtain the points shown with circles. The triangles, on the other hand, uses center‐to‐center angles. Our best‐fit determination of the input spectrum during R1 is used.

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