Extreme value distribution for gamma-ray-burst prompt data -- How unexpected was the BOAT event?
arXiv:2507.14041 · doi:10.1051/0004-6361/202555059
Abstract
Gamma-Ray Bursts (GRBs) are known to be unpredictable in time and position. A few (observationally) exceptional events have been observed, as GRB221009A that stands out for its fluence and peak flux, being orders of magnitude higher than what measured so far. Analyzing the observed fluence, peak flux or duration distributions typically requires one to assume some scenarios, and the consistency of the observed data with the predictions turns out to be an important model diagnostic. However, it is also of interest to model these distributions using general statistical properties that do not rely on specific model assumptions, allowing one to derive inferences only based on the consistency of the observed distributions with the hypothesis of one single population of events that generate them. We obtained fluences, peak fluxes and durations from the catalogues of GRBs observed by the CGRO-BATSE and Fermi-GBM instruments. We selected the extreme values in slots of equal duration and modelled their distributions by the generalized extreme value (GEV) formalism. The GEV distribution is a limit distribution naturally arising when the number of observations is large and is essentially independent of the phenomena producing the observed data. The distributions of extreme values for fluences, peak fluxes and durations are consistent with being extracted from a single population of events but the fluence and peak flux recorded for GRB221009A constitutes a striking exception. The probability to observe such an event, assuming it is a cosmological GRB, is low, with a median value of about one event per millennium for the fluence and about one event per century for the peak flux.
arXiv commentA&A, in press, includes editorial corrections
References in corpus (28)
- MCMC using Hamiltonian dynamics
- GRB Formation Rates inferred from the Spectral Peak Energy - Luminosity Relation
- The Ep,i - Eiso correlation in GRBs: updated observational status, re-analysis and main implications
- The Complete Spectral Catalog of Bright BATSE Gamma-Ray Bursts
- The Fermi GBM Gamma-Ray Burst Spectral Catalog: Four Years Of Data
- The Fourth Fermi-GBM Gamma-Ray Burst Catalog: A Decade of Data
- A new population of ultra-long duration gamma-ray bursts
- The 2nd Fermi GBM Gamma-Ray Burst Catalog: The First Four Years
- A complete sample of bright Swift Long Gamma-Ray Bursts: Sample presentation, Luminosity Function and evolution
- The 3rd Fermi GBM Gamma-Ray Burst Catalog: The First Six Years
- A long-duration gamma-ray burst with a peculiar origin
- JWST detection of heavy neutron capture elements in a compact object merger
- Gamma Ray Bursts in the comoving frame
- BATSE Observations of the Large-Scale Isotropy of Gamma-Ray Bursts
- GRB 221009A, The BOAT
- Fermi-GBM Discovery of GRB 221009A: An Extraordinarily Bright GRB from Onset to Afterglow
- The Konus-Wind catalog of gamma-ray bursts with known redshifts. I. Bursts detected in the triggered mode
- The Fermi GBM Gamma-Ray Burst Spectral Catalog: 10 Years of Data
- A Comprehensive Analysis of Fermi Gamma-ray Burst Data: III. Energy-Dependent T90 Distributions of GBM GRBs and Instrumental Selection Effect on Duration Classification
- The BATSE 5B Gamma-Ray Burst Spectral Catalog
- Properties of the extremely energetic GRB~221009A from Konus-WIND and SRG/ART-XC observations
- GRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst
- A Peculiarly Short-duration Gamma-Ray Burst from Massive Star Core Collapse
- The Gamma-ray Bursts fundamental plane correlation as a cosmological tool
- GRB 221009A: An ordinary nearby GRB with extraordinary observational properties
- Precision Prediction for the Cosmological Density Distribution
- On the modelling of the excesses of galaxy clusters over high-mass thresholds
- GRB 221009A and the Apparently Most Energetic Gamma-Ray Bursts