Light Curves (IMAGE) University of Copenhagen - Niels Bohr Institute Caption Seen here is the blue dot light curve (the brightness as a function of the time after the explosion) for the supernova associated with the super-long gamma-ray burst (GRB111209A). Also shown for comparison are the light curves for a normal envelope stripped supernova that is approximately 15 times weaker, an earlier supernova associated with a gamma-ray burst that is more than three times weaker and a so-called super luminous supernova that is even more extreme. The dark blue curve shows the result of a model where the energy for the supernova associated with GRB111209A comes from a braking magnetar. Credit (Johan Fynbo, NBI) Usage Restrictions (Credit: Johan Fynbo, NBI) License Licensed content Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.