activity
19952026
most citedFurther Study of the Gamma-Ray Bursts Duration Distribution

83 citations · 548 across the 28 of their papers we have counts for

collaborators

36 papers

astro-ph.HE2026

Correlation between X-ray and gamma data of Swift measurements

Istvan I. Racz, Lajos G. Balazs, Istvan Horvath +1

Several studies over the last two decades have used canonical correlation analysis (CCA) to study the relationships between main γ-ray (e.g. fluence, peak flux, and duration) and m…

astro-ph.CO2026

Spheroidal Resampling Analysis of High-Redshift Gamma-Ray Burst Spatial Densities

Istvan Horvath, Zsolt Bagoly, Lajos G. Balazs +6

Gamma-ray bursts (GRBs) are bright transient sources that can be observed at high redshift. They can therefore be used as tracers of the distant large-scale structure, although the…

astro-ph.CO2026★ 1 cited

Reanalysing large-scale structure using an updated gamma-ray burst spatial density approach

Istvan Horvath, Zsolt Bagoly, Jon Hakkila +6

In the past few decades, large universal structures have been found that challenge the homogeneity and isotropy expected in standard cosmological models. This study examines burst…

astro-ph.CO2025★ 4 cited

Scanning the Universe for Large-Scale Structures using Gamma-Ray Bursts

Istvan Horvath, Zsolt Bagoly, Lajos G. Balazs +5

In the past few decades, large universal structures have been found that challenge the homogeneity and isotropy expected in standard cosmological models. The largest of these, iden…

astro-ph.CO2023

Mapping the Universe with Gamma-Ray Bursts

Istvan Horvath, Zsolt Bagoly, Lajos G. Balazs +7

We explore large-scale cosmic structure using the spatial distribution of 542 gamma-ray bursts (GRBs) having accurately measured positions and spectroscopic redshifts. Prominent co…

astro-ph.HE2023

Some statistical remarks on GRBs jointly detected by Fermi and Swift satellites

Sandor Pinter, Lajos G. Balazs, Zsolt Bagoly +3

We made statistical analysis of the Fermi GBM and Swift BAT observational material, accumulated over 15 years. We studied how GRB parameters (T duration, fluence, peak flux)…