HETE-2 localization and observation of the gamma-ray burst GRB 020813

A bright, long gamma-ray burst (GRB) was detected and localized by the instruments on board the High Energy Transient Explorer 2 satellite (HETE-2) at 02:44:19.17 UTC (9859.17s UT) on 2002 August 13. The location was reported to the GRB Coordinates Network (GCN) about 4min after the burst. In the prompt emission, the burst had a duration of approximately 125s, and more than four peaks. We analyzed the time-resolved 2–400keV energy spectra of the prompt emission of GRB 020813 using the Wide Field X-Ray Monitor (WXM) and the French Gamma Telescope (FREGATE) in detail. We found that the early part of the burst (17–52s after the burst trigger) shows a depletion of low-energy photons below about 50keV. It is difficult to explain the depletion by either synchrotron self-absorption or Comptonization. One possibility is that the low-energy depletion may be understood as a mixture of “jitter” radiation with the usual synchrotron radiation component.

[1]  Gregory Y. Prigozhin,et al.  Global Characteristics of X-Ray Flashes and X-Ray-Rich Gamma-Ray Bursts Observed by HETE-2 , 2005 .

[2]  J. G. Jernigan,et al.  Global characteristics of X-ray flashes and X-ray rich GRBs observed by HETE-2 , 2004, astro-ph/0409128.

[3]  Y. Urata,et al.  Multiband Optical Follow-up Observations of GRB 020813 at the Kiso and Bisei Observatories , 2003, astro-ph/0308113.

[4]  D. Fugazza,et al.  Optical and NIR observations of the afterglow of GRB 020813 , 2003, astro-ph/0304171.

[5]  S. R. Kulkarni,et al.  Optical Spectropolarimetry of the GRB 020813 Afterglow , 2002, astro-ph/0212554.

[6]  Yuji Shirasaki,et al.  Performance of the wide-field x-ray monitor on board the High-Energy Transient Explorer 2 , 2000, Astronomical Telescopes and Instrumentation.

[7]  M. Rees,et al.  Compton dragged gamma‐ray bursts: the spectrum , 2000, astro-ph/0002049.

[8]  M. Medvedev Theory of “Jitter” Radiation from Small-Scale Random Magnetic Fields and Prompt Emission from Gamma-Ray Burst Shocks , 2000, astro-ph/0001314.

[9]  M. Feroci,et al.  Prompt and Delayed Emission Properties of Gamma-Ray Bursts Observed with BeppoSAX , 1999, astro-ph/9911228.

[10]  J. Chiang,et al.  Spectral Energy Distributions of Gamma-Ray Bursts Energized by External Shocks , 1999, astro-ph/9910472.

[11]  M. Rees,et al.  Compton-dragged Gamma-Ray Bursts Associated with Supernovae , 1999, The Astrophysical journal.

[12]  R. Preece,et al.  The BATSE Gamma-Ray Burst Spectral Catalog. I. High Time Resolution Spectroscopy of Bright Bursts Using High Energy Resolution Data , 1999, astro-ph/9908119.

[13]  Abraham Loeb,et al.  Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray Burst Sources , 1999, astro-ph/9904363.

[14]  T. Piran Gamma-ray bursts and the fireball model , 1998, astro-ph/9810256.

[15]  R. Preece,et al.  The Synchrotron Shock Model Confronts a “Line of Death” in the BATSE Gamma-Ray Burst Data , 1998, astro-ph/9808184.

[16]  T. Piran,et al.  Spectra and Light Curves of Gamma-Ray Burst Afterglows , 1997, astro-ph/9712005.

[17]  A. Crider,et al.  Physical Model of Gamma-Ray Burst Spectral Evolution , 1997 .

[18]  M. Tavani A Shock Emission Model for Gamma-Ray Bursts. II. Spectral Properties , 1996 .

[19]  E. Fenimore,et al.  Gamma-Ray Burst Peak Duration as a Function of Energy , 1995, astro-ph/9504075.

[20]  D. Palmer,et al.  BATSE observations of gamma-ray burst spectra. I: Spectral diversity , 1993 .

[21]  W. Priedhorsky,et al.  Prevalent properties of gamma-ray burst variability , 1993 .

[22]  H. Janka,et al.  GAMMA-RAY BURST AND AFTERGLOW ASTRONOMY 2001 , 2003 .

[23]  G. Rybicki,et al.  Radiative processes in astrophysics , 1979 .