Speaker
Dr
Stefano Covino
(INAF / Brera)
Description
The availability of a new generation of instruments with capabilities to observe at high or very-high energies open an exciting perspective for GRB studies. The very large accessible energy band, including lower energy observations (soft X-rays down to optical and radio), will allow a reliable modeling of the GRB spectra both during the prompt phase and the afterglows. These information can then allow us to constrain the emission processes and therefore solve some of the hottest issue in GRB research.
Author
Dr
Stefano Covino
(INAF / Brera)
