Skip to main content
Introducing Einstein Probe, Astro Flavored Markdown, and Notices Schema v4.0.0. See news and announcements

GCN Circular 833

Subject
GRB000926: X-ray afterglow by BeppoSAX: revised fluxes (fwd)
Date
2000-10-06T14:50:33Z (24 years ago)
From
Luigi Piro at IAS/CNR Frascati <piro@ias.rm.cnr.it>
L. Piro (BeppoSAX Mission Scientist, IAS/CNR Roma) & L. A. Antonelli (OaR)
report on behalf of the BeppoSAX team:


We have found an error in the application of a conversion factor which
underestimates the fluxes distributed in GCN n.832

The correct value of the average flux (at T=29.25) is

 F(1.6-10 keV)= (2.6+\-0.6) 10^-13 erg/cm2/s

We have also carefully checked different background subtraction methods,
finding that the corresponding systematic effect amouts to less than about
15%. This has been included in the flux error quoted above.

All the other results on the fading behaviour and on the spectral
shape presented in GCN 832 remain unaffected.
Looking for U.S. government information and services? Visit USA.gov