Correlation between intrinsic peak luminosity and spectral peak energy for energetic Fermi GRBs

Feraol Fana Dirirsa, Soebur Razzaque

Research output: Contribution to journalConference articlepeer-review

Abstract

We select energetic GRBs detected by Fermi-LAT/GBM with known redshift and compute the correlation between the intrinsic peak luminosity (Liso) and peak energy (Ei,p) of the νFν energy spectrum, known as the Yonetoku relation, in the 1 keV–10 MeV and 1 keV–30 MeV energy ranges. This correlation has the potential to make GRBs standard candles, similar to type Ia supernovae, but extending to high redshift. We explore parameters of the Lambda-Cold-Dark-Matter cosmological model at high redshift using Yonetoku relation for our sample of GRBs.

Original languageEnglish
Article number002
JournalProceedings of Science
Volume319
Publication statusPublished - 2017
Event5th Annual Conference on High Energy Astrophysics in Southern Africa, HEASA 2017 - Johannesburg, South Africa
Duration: 4 Oct 20176 Oct 2017

ASJC Scopus subject areas

  • Multidisciplinary

Fingerprint

Dive into the research topics of 'Correlation between intrinsic peak luminosity and spectral peak energy for energetic Fermi GRBs'. Together they form a unique fingerprint.

Cite this