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Prospects for Gamma-Ray Burst Afterglow Discovery with the Eric and Wendy Schmidt Observatory System

  • Authors: James Freeburn, Dougal Dobie, Akash Anumarlapudi, Igor Andreoni, Brendan O'Connor, Eric Burns, Jonathan Carney, Hank Corbett, Michael W. Coughlin, Adam Goldstein, Anna Tartaglia, V. Ashley Villar

James Freeburn et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 6.

An example of an LGRB afterglow model with a prominent, early reverse shock, showing simulated observations at the base cadence (left panel), 15 minute coadds (center panel), and 60 minute and nightly coadds (right panel). The injected light curve is shown with solid lines, and its parameters are: z = 1.47, Eiso = 7.98 × 1053 erg, n0 = 0.64 cm−3, θc = 12﹩\mathop{.}\limits^{{\unicode{x000b0}}}﹩42, p = 2.58, ﹩\mathrm{log}{\epsilon }_{e}=-1.02﹩, ﹩\mathrm{log}{\epsilon }_{B}=-4.83﹩, tj = 3.24 s, ﹩\mathrm{log}{R}_{b}=3.85﹩ and AV = 0.24.

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