Methods. Multi-wavelength follow-up observations were performed on the afterglow of GRB 080413B. X-ray emission was detected by the X-ray telescope onboard the Swift satellite and obtained from the public archive. Optical and near-infrared photometry was performed with the seven-channel imager GROND mounted at the MPG/ESO 2.2 m telescope and additionally with the REM telescope, both in La Silla, Chile. The light curve model was constructed using the obtained broad-band data.
Results. The broad-band light curve of the afterglow of GRB 080413B is well fitted with an on-axis two-component jet model. The narrow ultra-relativistic jet is responsible for the initial decay, while the rise of the moderately relativistic wider jet near its deceleration time is the cause of the rebrightening of the light curve. The later evolution of the optical/NIR light curve is then dominated by the wide component, the signature of which is almost negligible in the X-ray wavelengths. These components have opening angles of θn ~ 1.7° and θw ~ 9°, and Lorentz factors of Γn > 188 and Γw ~ 18.5. We calculated the beaming-corrected energy release to be Eγ = 7.9 × 1048 erg.
- ISM: jets and outflows, gamma rays: general, X-rays: individuals: GRB 080413B, Astrophysics - High Energy Astrophysical Phenomena