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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 4.

Detection efficiency and rates of afterglow detection with DSA and Argus from GRBs detected with a variety of GRB energy bands and sensitivities. We assume Ωγ = 3π and Dγ = 0.95. Top panel: the afterglow detection efficiency with GRB detector sensitivity. Bottom panel: afterglow detection rates with GRB detector sensitivity. The afterglow detection efficiencies from Argus and DSA for GRBs detected with Fermi/GBM are plotted as black horizontal lines for comparison.

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