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Introduzione
Contents
Contents
List of Figures
List of Tables
The BeppoSAX Gamma Ray Burst Monitor experiment
The BeppoSAX satellite
Mission overview
The scientific payload
Data formats and data reduction software
The Gamma-Ray Burst Monitor experiment
Inorganic scintillator detectors
The Phoswich Detection System
The Gamma-Ray Burst Monitor
GRBM scientific data
GRBM on-ground calibrations
On-ground performance tests of GRBM detectors
Functional tests on plain crystals
Detectors calibrations with PDS experiment integrated
On-ground GRBM calibrations performed after spacecraft integration
Radioactive sources
Measurement set-up and strategy
Monitoring of spurious contributions
Calibrations database and preliminary analysis
Ratemeters data
Energy spectra
Background
Sources calibration and spurious contributions
GRBM detectors response functions
Gamma-ray spectroscopy with inorganic scintillators
Interaction of gamma radiation with matter
Spectral response of real scintillators
Response matrix and spectral data fitting
Building the response matrix
Spectral fitting
Response in the GRBM and AC ratemeters bands
On-axis efficiency
Analytical interpolation of LS1 and LS3 efficiency angular dependency
Interpolation of LS2 and LS4 efficiencies
Spectral response matrices of LS1 and LS3
Channel to energy conversion and energy resolution
Spectral shape modeling
Thresholds effects
Standardization of response matrices formats
Expected counts spectra for different source photon spectra
Comparison between calibrations results and preliminary Monte Carlo simulations
The Monte Carlo model
Simulation of on-ground measurements and comparison with the calibrations data
The in-flight data: source detection, data analysis and response functions verification
GRBM in-flight performances
In-orbit background
Background level and variations in the GRBM and AC ratemeters
Background spectral properties
Gamma-ray burst detection
Detection of sources with the Earth occultation technique
Derivation of flux and spectral evolution from 1 s ratemeters
Energy spectra analysis
Source direction
Dead time and counter recycling corrections
Dead time
Counters recycling
Systematics due to uncertainties in detectors efficiencies
Data reduction and analysis software
Data reduction software
Raw data processing
FOT data processing
Specific GRBM data analysis software
GRBM data analysis with standard softwares
In-flight verification of the response functions
Measurements of Crab nebula flux and spectrum
The Crab Nebula as a standard candle
Crab Nebula flux and photon index from the 1 s ratemeters
Crab Nebula 240 channels spectrum
Comparison with CGRO/BATSE results
The BATSE experiment and GRB catalogue
Simultaneous detection of GRBM and BATSE
Comparison between GRBM and BATSE results
WFC and GRBM joint data analysis and intercalibration with Crab spectrum
WFC + GRBM detections of GRB
Data analysis and intercalibration
Astrophysics of Gamma-Ray Bursts with the GRBM
Astronomy of cosmic gamma-ray burst
Observations
Morphology and duration distribution
Angular distribution
Peak intensity distribution
Spectral properties
Theory
Local origin
Extended galactic halo
Cosmological origin
The 1997 breakthrough in GRB astronomy: BeppoSAX results
Pre-SAX experimental scenario
Afterglow discovery
BeppoSAX detection and X-ray follow-up observation
Optical follow-up observation
Other wavelengths
The first measurement of a GRB distance: GRB970508
Further developments
The redshift and GRB971214
The intriguing GRB980425 and the Supernova Connection
Broad band spectral analysis of GRB with the GRBM
The GRBM + WFC events database
Average spectra
Spectral evolution
GRB960720: very fast spectral evolution
GRB970111: high statistics
GRB970228: the GRB-afterglow connection
GRBM observations and spectral analysis of
SGR1900+14
Soft Gamma Repeaters
SGR1900+14
GRBM Observation
Spectral Analysis
Time-averaged Analysis
Time-resolved Analysis
Discussion
Conclusions and future perspectives
Summary of Thesis work results
Work in progress
Future perspectives
References
Thesis work related publications
GRBM description, calibration, response function and data analysis
Astrophysical applications of GRBM response functions and data analysis techniques
GRB afterglows specific papers
Prompt GRB follow-up and SGR detections: IAU Circulars
Lorenzo Amati
8/30/1999