Statistical analysis of RHESSI GRB database
J. Ripa, R. Hudec, A. Meszaros, W. Hajdas, C. Wigger
TL;DR
This paper analyzes the RHESSI GRB database to study the distribution of durations and hardness ratios, providing insights into gamma-ray burst characteristics.
Contribution
It presents the first statistical analysis of the RHESSI GRB database focusing on duration and hardness ratio distributions.
Findings
Duration distribution shows bimodal pattern.
Hardness ratio varies with burst duration.
Sample includes 228 GRBs.
Abstract
The Gamma-ray burst (GRB) database based on the data by the RHESSI satellite provides a unique and homogeneous database for future analyses. Here we present preliminary results on the duration and hardness ratio distributions for a sample of 228 GRBs observed with RHESSI.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGamma-ray bursts and supernovae · Astronomical Observations and Instrumentation · Astronomy and Astrophysical Research