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First Results from the PanRadio Gamma-Ray Burst Collaboration: The 400-day Afterglow of GRB 230815A

  • Authors: James K. Leung, Gemma E. Anderson, Alexander J. van der Horst, Claire Morley, Benjamin Schneider, Fabio De Colle, Om Sharan Salafia, Giancarlo Ghirlanda, Sarah I. Chastain, Adelle J. Goodwin, Ashna Gulati, Lauren Rhodes, Stuart D. Ryder, Ashley A. Chrimes, Valerio D'Elia, Mathieu de Bony de Lavergne, Massimiliano De Pasquale, Antonio de Ugarte Postigo, Dieter H. Hartmann, Benjamin P. Gompertz, Andrew J. Levan, Tara Murphy, Gavin P. Rowell, Thomas D. Russell, Fabian Schüssler, Rhaana L. C. Starling, Nial R. Tanvir, Susanna D. Vergani, Ralph A. M. J. Wijers

James K. Leung et al 2026 The Astrophysical Journal Letters 997 .

  • Provider: AAS Journals

Caption: Figure 3.

Broadband SED of GRB 230815A, showing two temporal snapshots at approximately 0.5 (red) and 1.5 (blue) days postburst. The light gray points represent data from later epochs, after 1.5 days postburst. Radio detections are shown with circular markers, near-infrared detections are shown with star markers, and all upper limits are shown with inverted triangular markers. The X-ray spectrum (dark red filled) is extrapolated to the near-infrared part of the spectrum (light red filled) using a photon index of ﹩{\rm{\Gamma }}=1.9{4}_{-0.10}^{+0.11}﹩, where the shaded region corresponds to a 68% confidence interval. The slopes between various data points in each spectral snapshot are annotated next to the corresponding dashed guide lines.

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