Image Details

Choose export citation format:

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 3.

Distribution of simulated depths in Argus g and r-band for a the baseline cadence in addition to observations stacked at 15 minute, 1 hr, and day duration intervals. The y-axis shows the density of observations at each depth bin and cadence, in arbitrary units. The baseline cadence includes second-cadence observations in bright time with median depths of g = 16.8 and r = 16.9 AB mag and minute-cadence data in dark and gray time with depths of g = 20.5 and r = 20.2 AB mag.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse