Webbläsaren som du använder stöds inte av denna webbplats. Alla versioner av Internet Explorer stöds inte längre, av oss eller Microsoft (läs mer här: * https://www.microsoft.com/en-us/microsoft-365/windows/end-of-ie-support).

Var god och använd en modern webbläsare för att ta del av denna webbplats, som t.ex. nyaste versioner av Edge, Chrome, Firefox eller Safari osv.

Default user image.

Sofia Feltzing

Professor

Default user image.

GRB 030227 : The first multiwavelength afterglow of an INTEGRAL GRB

Författare

  • A. J. Castro-Tirado
  • J. Gorosabel
  • S. Guziy
  • D. Reverte
  • J. M. Castro Cerón
  • A. de Ugarte Postigo
  • N. Tanvir
  • S. Mereghetti
  • A. Tiengo
  • J. Buckle
  • R. Sagar
  • S. B. Pandey
  • V. Mohan
  • N. Masetti
  • F. Mannucci
  • Sofia Feltzing
  • Ingemar Lundström
  • H. Pedersen
  • C. Riess
  • S. Trushkin
  • J. Vílchez
  • N. Lund
  • S. Brandt
  • S. Martínez Núñez
  • V. Reglero
  • M. D. Pérez-Ramírez
  • S. Klose
  • J. Greiner
  • J. Hjorth
  • L. Kaper
  • E. Pian
  • E. Palazzi
  • M. I. Andersen
  • A. Fruchter
  • J. P. U. Fynbo
  • B. L. Jensen
  • C. Kouveliotou
  • J. Rhoads
  • E. Rol
  • P. M. Vreeswijk
  • R. A. M. J. Wijers
  • E. van den Heuvel

Summary, in English

We present multiwavelength observations of a gamma-ray burst detected byINTEGRAL (GRB 030227) between 5.3 hours and ~ 1.7days after the event. Here we report the discovery of a dim opticalafterglow (OA) that would not have been detected by many previoussearches due to its faintess (R ~ 23). This OA was seen to declinefollowing a power law decay with index alpha R = -0.95 +/-0.16. The spectral index beta_ opt/NIR yielded -1.25 +/- 0.14. Thesevalues may be explained by a relativistic expansion of a fireball (withp = 2.0) in the cooling regime. We also find evidence for inverseCompton scattering in X-rays.Based on observations with INTEGRAL, an ESA project with instruments andscience data centre funded by ESA member states (especially the PIcountries: Denmark, France, Germany, Italy, Switzerland, Spain), CzechRepublic and Poland, and with the participation of Russia and the USA.Also partially based on observations collected by the Gamma-Ray BurstCollaboration at ESO (GRACE) at the European Southern Observatory, Chile(ESO Large Programme 165.H-0464).

Avdelning/ar

  • Astronomi - Har omorganiserats

Publiceringsår

2003

Språk

Engelska

Sidor

315-319

Publikation/Tidskrift/Serie

Astronomy & Astrophysics

Volym

411

Issue

1

Dokumenttyp

Artikel i tidskrift

Förlag

EDP Sciences

Ämne

  • Astronomy, Astrophysics and Cosmology

Nyckelord

  • gamma rays: bursts
  • techniques: photometric
  • cosmology: observations

Status

Published

ISBN/ISSN/Övrigt

  • ISSN: 0004-6361