Published May 22, 2008 | Version v1
Journal article

Development of A New Background Reduction Method for WXM/HETE-2 and Its Application for Bright GRB Spectra

  • 1. Department of Physics and Mathematics, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 229-8558 (Japan)
  • 2. Institute of Physical and Chemical Research, 2-1 Hirosawa, Wako, Saitama 351-0198 (Japan)
  • 3. Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551 (Japan)
  • 4. ISAS/JAXA, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510 (Japan)
  • 5. National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588 (Japan)
  • 6. Center for Space Research, MIT, 77 Vassar Street, Cambridge, MA 02139-4307 (United States)

Description

HETE-2 detected gamma-ray bursts (GRBs) since its launch on 9 October 2000. For spectral analyses using data of WXM on-board HETE-2, background spectra are conventionally obtained with time regions before and/or after prompt emission. In some cases, the background spectra change during the prompt emission and/or the downlink trouble causes a loss of data around the prompt emission. If this is the case, the problem seems to lie in the fact that the conventional method cannot obtain correct background spectra. To make more appropriate background spectra, we develop a new analysis method using mask patterns of the WXM. The background spectra are estimated with shaded regions by the WXM mask pattern using the prompt emission data. Our new method might obtain a reliable result for a spectrum of GRB 030329. In this paper, we introduce our new analysis method and show a preliminary spectral result

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1000
Journal Issue
1
Journal Page Range
p. 174-177
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Santa Fe conference on gamma-ray bursts 2007
Dates
5-9 Nov 2007
Place
Santa Fe, NM (United States)

Optional Information

Notes
(c) 2008 American Institute of Physics