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Astron. Astrophys. Suppl. Ser.
Volume 138, Number 3, September 1999
Gamma-Ray Bursts in the Afterglow Era Contents Rome, November 3-6, 1998
Page(s) 567 - 568
Published online 15 September 1999
DOI: 10.1051/aas:1999355

Astron. Astrophys. Suppl. Ser. 138, 567-568

Gamma-ray burst afterglow observations using AXAF and ACIS

G.P. Garmire

Pennsylvania State University, 525 Davey Lab, University Park, PA 16802, U.S.A.

Received December 18, 1998; accepted March 10, 1999


With the successful launch of AXAF next summer, it will be possible to observe the X-ray afterglow from gamma-ray bursts with much improved positional accuracy ($\sim 1$ arcsec) and sensitivity (2-10 keV, $1.5\ 10^{-14}~{\rm ergs/cm}^2/{\rm s}$ in 10 ksec). A typical burst afterglow should be observable within about 10 hours after the position has been determined by BeppoSAX or any other satellite capable of determining the position to within about 5 arcmin and provide about 1000 counts in a 10 ksec integration using the ACIS on AXAF. To constrain the decrease of intensity with time, using existing data from BeppoSAX and ASCA, the burst should produce a measurable flux for up to about 4 months after the gamma-ray event for an observing time of about 40 ksec, if a simple extrapolation of the observed fall-off with time is assumed. Depending upon a number of assumptions, there is a slight possibility of observing iron lines from the gas immediately surrounding the gamma-ray burst source using a long exposure (>100 ksec).

Key words: gamma-ray bursts

Copyright The European Southern Observatory (ESO)

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