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Polarimetry and Photometry of Gamma-Ray Bursts with RINGO2

  • Authors: I. A. Steele, D. Kopač, D. M. Arnold , R. J. Smith, S. Kobayashi, H. E. Jermak, C. G. Mundell, A. Gomboc, C. Guidorzi, A. Melandri, and J. Japelj

2017 The Astrophysical Journal 843 143.

  • Provider: AAS Journals

Caption: Figure 10.

GRB 110205A, GRB 110726A, GRB 120119A, and GRB 120308A for which the light curves show definite structure. The Beuermann and PL components defined in Table 4 are plotted individually as dotted lines, and the final r-band model fit (the summation of the multiple components) is plotted as a solid line. To more easily compare the light-curve shape between filters by eye, the model is plotted multiple times offset to align with the non-﹩r^{\prime} ﹩ band filters and plotted as a dashed line. The steep rise for GRB 110205A and GRB 120308A indicates the presence of the reverse-shock component in the afterglow.

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