Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-07-08
Astron.Astrophys. 426 (2004) 415-423
Astronomy and Astrophysics
Astrophysics
10 pages, 8 figures, accepted for pubblication in Astronomy & Astrophysics, main journal
Scientific paper
10.1051/0004-6361:20047146
We report on the X-ray observations of the X-ray flash (XRF) which occurred on 2002 April 27, three days before BeppoSAX was switched off. The event was detected with the BeppoSAX Wide Field Cameras but not with the Gamma ray Burst Monitor. A follow-up observation with the BeppoSAX Narrow Field Instruments was soon performed and a candidate afterglow source was discovered. We present the results obtained. We also include the results obtained from the observations of the XRF field with the Chandra X-ray satellite. The spectral analysis of the prompt emission shows that the peak energy of the EF(E) spectrum is lower than 5.5 keV, with negligible spectral evolution. The X-ray afterglow spectrum is consistent with a power law model with photon index of about 2, while the 2-10 keV flux fades as a power law with a decay index -1.33. Both these indices are typical of GRBs. A very marginal excess around 4.5-5 keV is found in the afterglow spectrum measured by BeppoSAX . As for many GRBs, the extrapolation of the 2-10 keV fading law back to the time of the prompt emission is consistent with the X-ray flux measured during the second part of the event. We estimate a possible range of values of the redshift and discuss our results in the light of current models of XRFs.
Amati Lorenzo
Antonelli Lucio Angelo
Capalbi Milvia
Costa Edgar
Feroci Marco
No associations
LandOfFree
Prompt and afterglow X-ray emission from the X-Ray Flash of 2002 April 27 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Prompt and afterglow X-ray emission from the X-Ray Flash of 2002 April 27, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Prompt and afterglow X-ray emission from the X-Ray Flash of 2002 April 27 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-221650