The INTEGRAL/IBIS scientific data analysis

@article{Goldwurm2003TheIS,
title={The INTEGRAL/IBIS scientific data analysis},
author={A. Goldwurm and P. David and Luigi Foschini and Alexandra Gros and Philippe Laurent and Aymeric Sauvageon and A J Bird and Laurent Lerusse and N. Produit SApCEA-Saclay and France IASFCNR-Bologna and Italy Southampton Un. and UK ISDC-Versoix and Switzerland.},
journal={Astronomy and Astrophysics},
year={2003},
volume={411}
}
• Published 1 November 2003
• Physics
• Astronomy and Astrophysics
The gamma-ray astronomical observatory INTEGRAL, succesfully launched on 17th October 2002, carries two large gamma-ray telescopes. One of them is the coded-mask imaging gamma-ray telescope onboard the INTEGRAL satellite (IBIS) which provides high-resolution ( ≈ 12 ' ) sky images of $29^{\circ}\times29^{\circ}$ in the energy range from 15 keV to 10 MeV with typical on-axis sensitivity of ≈ 1 mCrab at 100 keV (3 σ , 10 6  s exposure). We report here the general description of the IBIS coded-mask…
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References

SHOWING 1-10 OF 22 REFERENCES

IBIS: The Imager on-board INTEGRAL

• Physics
• 2003
The IBIS telescope is the high angular resolution gamma-ray imager on-board the INTEGRAL Observatory, suc- cessfully launched from Baikonur (Kazakhstan) the 17th of October 2002. This medium size ESA

The INTEGRAL IBIS/ISGRI System Point Spread Function and source location accuracy

• Physics
• 2003
The imager on board INTEGRAL (IBIS) presently provides the most detailed sky images ever obtained at energies above 30 keV. The telescope is based on a coded aperture imaging system which allows to

In-flight calibrations of IBIS/PICsIT ⋆

• Physics
• 2003
PICsIT (Pixellated Imaging CaeSium Iodide Telescope) is the high energy detector of the IBIS telescope on-board the INTEGRAL satellite. It consists of 4096 independent detection units,0.7 cm 2 in

The SIGMA/Granat Telescope: Calibration and Data Reduction

• Physics
• 2001
The SIGMA Telescope was a French experiment, designed to provide high-resolution images in the hard X-ray and soft γ-ray band (35-1300 keV). It featured a coded mask, a NaI(Tl) position-sensitive

ISGRI: The INTEGRAL soft gamma-ray imager

• Physics
• 2003
For the first time in the history of high energyastronomy, a large CdTe gamma-ray camera is operating in space. ISGRI is the low-energy camera of the IBIS telescope on board the INTEGRAL satellite.

IBIS/PICsIT in-flight performances

• Physics
• 2003
PICsIT (Pixellated Imaging CaeSium Iodide Telescope) is the high energy detector of the IBIS telescope on-board the INTEGRAL satellite. PICsIT operates in the gamma-ray energy range between 175 keV

The INTEGRAL mission

• C. Winkler
• Physics
SPIE Astronomical Telescopes + Instrumentation
• 2003
INTEGRAL, the International Gamma-Ray Astrophysics Laboratory, to be launched in 2001, is the second medium-size scientific mission (M2) of the ESA long term programme “Horizon 2000”. INTEGRAL

In-flight calibration of the ISGRI camera

• Physics
• 2003
ISGRI, the IBIS low energy camera (15 keV - 1 MeV) on board INTEGRAL, is the first large CdTe gamma-ray imager in orbit. We present here an overview of the ISGRI in-flight calibrations performed

Systematic effects induced on IBIS detectors by background and inhomogeneity of the spatial response

• Physics
• 2003
The spatial distribution of the background events may affect the source detection capability of IBIS at high energies (>200 keV) for both ISGRI and PICsIT layers. The observed background is found to

Coded aperture imaging in X- and gamma-ray astronomy

• Physics
• 1987
Coded aperture imaging in high energy astronomy represents an important technical advance in instrumentation over the full energy range from X- to γ-rays and is playing a unique role in those