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GRB 041219A: Its host galaxy and its broad-band prompt optical-to-gamma-ray emission

  • Diego Götz
  • , Stefano Covino
  • , Romain Hascoët
  • , Alberto Fernández-Soto
  • , Frédéric Daigne
  • , Robert Mochkovitch
  • , Paolo Esposito

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

GRB 041219A is one of the longest and brightest gamma-ray bursts (GRBs) ever observed. It was discovered by the INTEGRAL satellite, and, thanks to a precursor happening about 300 s before the bulk of the burst, ground based telescopes were able to catch the rarely-observed prompt emission in the optical and in the near-infrared bands. Here we present the late-time multi-band near-infrared imaging data, collected at the CFHT, that allowed us to identify the host galaxy of the GRB as an under-luminous, irregular galaxy of ∼ 5 × 109M at best-fit redshift of z = 0.31 -0.26+0.54. In addition we model the broad-band prompt optical to γ-ray emission of GRB 041219A within the internal shock model, where we were able to reproduce the spectra and light curve invoking the synchrotron emission of relativistic electrons accelerated by a series of propagating shock waves inside a relativistic outflow.

Original languageEnglish
Title of host publicationGamma Ray Bursts 2010, GRB 2010
Pages261-264
Number of pages4
DOIs
Publication statusPublished - 12 Sept 2011
Externally publishedYes
EventGamma Ray Bursts 2010, GRB 2010 - Annapolis, MD, United States
Duration: 1 Nov 20104 Nov 2010

Publication series

NameAIP Conference Proceedings
Volume1358
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Conference

ConferenceGamma Ray Bursts 2010, GRB 2010
Country/TerritoryUnited States
CityAnnapolis, MD
Period1/11/104/11/10

Keywords

  • Bursts
  • Galaxies
  • Gamma-rays
  • Observations
  • Photometry

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