Smoothly Broken Power Law Spectra of Gamma-Ray Bursts

Simple item page
dc.creatorRyde, Felix
dc.date1998-11-30
dc.date.accessioned2026-07-07T02:29:21Z
dc.date.available2026-07-07T02:29:21Z
dc.descriptionA five-parameter expression for a smoothly broken power law is presented. It is used to fit Gamma-Ray Burst (GRB) spectra observed by BATSE. The function is compared to previously used four-parameter functions, such as a sharply broken power law and the Band et al. (1993) function. The presented function exists as a WINGSPAN routine at http://www.astro.su.se/~felix/wing.html
dc.descriptionIn the proc. of the 3rd INTEGRAL Workshop: The Extreme Universe
dc.identifierhttps://arxiv.org/abs/astro-ph/9811462
dc.identifierhttp://arxiv.org/abs/astro-ph/9811462
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13442
dc.subjectAstrophysics
dc.titleSmoothly Broken Power Law Spectra of Gamma-Ray Bursts
dc.typetext

Files

Collections

arXiv