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The 2175 Å Extinction Feature in the Optical Afterglow Spectrum of GRB 180325A at z = 2.25

  • Authors: T. Zafar, K. E. Heintz, J. P. U. Fynbo, D. Malesani, J. Bolmer, C. Ledoux, M. Arabsalmani, L. Kaper, S. Campana, R. L. C. Starling, J. Selsing, D. A. Kann, A. de Ugarte Postigo, T. Schweyer, L. Christensen, P. Møller, J. Japelj, D. Perley, N. R. Tanvir, P. D'Avanzo, D. H. Hartmann, J. Hjorth, S. Covino, B. Sbarufatti, P. Jakobsson, L. Izzo, R. Salvaterra, V. D'Elia, and D. Xu

2018 The Astrophysical Journal Letters 860 L21.

  • Provider: AAS Journals

Caption: Figure 2.

Observer-frame afterglow SED of GRB 180325A. Black circles indicate the Swift X-ray data. The binned (for visual purposes) blue, green, and red data points (with 1σ errors) correspond to the UVB, VIS, and NIR VLT/X-shooter spectra, respectively. GROND observations are represented by black squares. The black solid and dashed lines show the best-fit dusty+absorbed and intrinsic spectral model, respectively. Inset: the black line shows the absolute extinction curve, and the gray shaded area materializes the associated 1σ uncertainty. The X-shooter spectra are indicated by cyan curves. The red dashed line corresponds to the mean MW curve from Fitzpatrick & Massa (2007).

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