CORDIS Project
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This project investigates gamma-ray bursts, which are powerful cosmic explosions, to enhance understanding of the early Universe and star formation. It involves training in optical afterglow spectroscopy and multi-wavelength studies of gamma-ray burst afterglows.
Gamma-ray bursts (GRBs) are cosmic, stellar explosions, that emit a typical amount of energy of 10^51 erg in gamma-rays on short time scales of 0.1 to 100 seconds.
The prompt emission in gamma-rays is followed by a longer-lasting afterglow, which can be detected in all wavelength ranges from radio, optical, to X- and gamma-rays up to several days after the explosion.
The large energy release and high luminosity of GRBs and their afterglows make them ideal probes for studying the early Universe a…
KOBENHAVNS UNIVERSITET
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