GCN Circular 5211
Subject
GRB 060602A: Swift-BAT Refined Analysis: Correction
Date
2006-06-04T02:13:48Z (18 years ago)
From
Takanori Sakamoto at NASA/GSFC <takanori@milkyway.gsfc.nasa.gov>
T. Sakamoto (GSFC/ORAU) on behalf of the Swift-BAT team:
There is an error in the 1-s peak photon flux reported in
Sakamoto et al. (GCN Circular 5206). Due to hard and weak
nature of the burst, only the 90% upper limit of 0.5 ph/cm2/s
is possible to constrain from a power-law fit.
We apologize for this mistake. We thank Kazutaka Yamaoka for
pointing it out.