A comparison of the fluences and photon peak fluxes for the Swift and RHESSI gamma-ray bursts
D. Huja, J. Ripa, A. Meszaros

TL;DR
This paper compares the fluences and photon peak fluxes of gamma-ray bursts detected by Swift and RHESSI satellites to analyze their observational differences.
Contribution
It provides a graphical comparison of GRB fluences and peak fluxes between two major gamma-ray observatories, highlighting their measurement differences.
Findings
Differences in fluence measurements between Swift and RHESSI.
Variations in photon peak fluxes observed by the two satellites.
Insights into the detection capabilities of each satellite.
Abstract
Fluences and photon peak fluxes of the gamma-ray bursts (GRBs) detected by the Swift and RHESSI satellites are graphically compared.
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Taxonomy
TopicsGamma-ray bursts and supernovae
