Published April 14, 2003
| Version v1
Journal article
Localization of GRBs by Bayesian analysis of data from the HETE WXM
- 1. Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States)
Description
We describe a new method of transient point source localization for coded-aperture X-ray detectors that we have applied to data from the HETE Wide-Field X-Ray Monitor (WXM). The method is based upon the calculation of the likelihood function and its interpretation as a probability density for the transient source location by an application of Bayes' Theorem. The method gives a point estimate of the source location by finding the maximum of this probability density, and credible regions for the source location by choosing suitable contours of constant probability density. We describe the application of this method to data from the WXM, and give examples of GRB localizations which illustrate the results that can be obtained using this method
Additional details
Identifiers
- DOI
- 10.1063/1.1579305;
- arXiv
- arXiv:astro-ph/0210429v1;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 662
- Journal Issue
- 1
- Journal Page Range
- p. 76-78
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- International meeting on gamma ray burst and afterglow astronomy
- Dates
- 5-9 Nov 2001
- Place
- Woods Hole, MA (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35067904
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- APERTURES; COSMIC GAMMA BURSTS; DATA ANALYSIS; POINT SOURCES; PROBABILITY; RADIATION MONITORS; SATELLITES
- Descriptors DEC
- COSMIC RADIATION; IONIZING RADIATIONS; MEASURING INSTRUMENTS; MONITORS; OPENINGS; PRIMARY COSMIC RADIATION; RADIATION SOURCES; RADIATIONS
Optional Information
- Notes
- (c) 2003 American Institute of Physics
- Collaborations
- HETE Science Team