Published December 2007 | Version v1
Journal article

The Suzaku-swift joint observation of the early X-ray afterglow of GRB060105

  • 1. Saitama Univ., Dept. of Physics, Saitama (Japan)
  • 2. NASA/Goddard Space Flight Center, Greenbelt, MD (US)

Description

Results are presented of a Suzaku and Swift joint observation for an early X-ray afterglow of GRB 060105. The bright, long gamma-ray burst GRB 060105 triggered the Swift Burst Alert Telescope (BAT) at 06:49:28 on 5 January 2006 (T0). The Suzaku team commenced a pre-planned target of opportunity observation at 12:10 and continued till 12:00 on January 6. The X-ray flux faded during the observations from 6.8x10-9 erg s-1cm-2 to 1.5x10-13 erg s-1 cm-2 in the 2-10 keV energy band. Following the prompt emission and successive 'very steep decay', a 'shallow decay' was observed from T0 + 187 s to T0 + 1287 s. After an observation gap during T0 + (1.5-3) ks, an extremely early steep decay was observed in T0 + (4-30) ks. The steep decay exhibited decay indices of 2.3 - 2.4. This very early break, if it is a jet break, is the earliest case among X-ray afterglow observations, suggesting a very narrow jet whose opening angle is well below 1deg. (author)

Additional details

Publishing Information

Journal Title
Progress of Theoretical Physics, Supplement
Journal Issue
no.169
Journal Page Range
p. 3-6
ISSN
0375-9687

Conference

Title
The extreme universe in the Suzaku era
Acronym
SUZAKU 2006
Dates
4-8 Dec 2006
Place
Kyoto (Japan)

Optional Information

Notes
16 refs., 1 fig.