Image Details
Caption: Figure 8.
Comparison of the LGRB-derived formation rates with the SFR density from P. Madau & M. Dickinson (2014). Green points with black error bars denote the observational SFR data, while the dashed blue and red curves correspond to the best-fit double-break models for the full and non-ML GRB catalogs, respectively.
© 2026. The Author(s). Published by the American Astronomical Society.