Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1279..369m&link_type=abstract
DECIPHERING THE ANCIENT UNIVERSE WITH GAMMA-RAY BURSTS. AIP Conference Proceedings, Volume 1279, pp. 369-371 (2010).
Astronomy and Astrophysics
Astronomy
Gamma-Ray Sources (Astronomical), Astronomical Telescopes, X-Ray Sources (Astronomical), Gamma-Ray, X- And Gamma-Ray Telescopes And Instrumentation, X-Ray Sources, X-Ray Bursts
Scientific paper
The detailed study of the spectral evolution during the steep decay phase of early X-ray light curves of Gamma-ray Bursts (GRBs) is a very important task that can give us information on different emission components contributing to the prompt-to-afterglow transition. Time resolved spectral analysis of bright GRBs detected by Swift has shown that a good modeling of the early X-ray light curves can be obtained with Band or cut-off power-law broad band spectra with evolving parameters (e.g., decaying peak energy). We developed a procedure to simultaneously fit the temporal evolution of all the spectral parameters of a GRB during the prompt to afterglow transition based on the analysis of the Swift Burst Alert Telescope (BAT) and the Swift X-ray Telescope (XRT) count rate and hardness ratio light curves. The procedure has been tested on GRB 060614 and GRB 090618, two very peculiar bright GRB detected by Swift that show a long exponentially decaying tail with strong softening and peak energy crossing the XRT energy band.
Mangano Valeria
Sbarufatti Boris
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