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The INTEGRAL mission – an overview

Published online by Cambridge University Press:  12 May 2006

P. Kretschmar ,
C. Winkler ,
T. J.-L. Courvoisier ,
G. Di Cocco ,
R. Diehl ,
N. Gehrels ,
S. Grebenev ,
W. Hermsen ,
J. M. Mas-Hesse  and
F. Lebrun
...Show all authors
P. Kretschmar
Affiliation:
ESA-ESAC, P.O. Box 50727, 28080 Madrid, Spain
C. Winkler
Affiliation:
ESA-ESTEC, RSSD, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
T. J.-L. Courvoisier
Affiliation:
INTEGRAL Science Data Centre, Chemin d'Écogia 16, 1290 Versoix, Switzerland Geneva Observatory, Ch. des Maillettes, 1290 Sauverny, Switzerland
G. Di Cocco
Affiliation:
IASF/CNR, Sezione di Bologna, via Gobetti 101, 40129 Bologna, Italy
R. Diehl
Affiliation:
Max-Planck Institut fr extraterr. Physik, Postfach 1603, 85740 Garching, Germany
N. Gehrels
Affiliation:
NASA-GSFC, Code 661, Greenbelt, MD 20771, USA
S. Grebenev
Affiliation:
Space Research Institute, Profsoyuznaya 84/32, 117810 Moscow, Russia
W. Hermsen
Affiliation:
Space Research Institute, Profsoyuznaya 84/32, 117810 Moscow, Russia
J. M. Mas-Hesse
Affiliation:
SRON-Utrecht, Sorbonnelaan 2, 3584 CA Utrecht, The Netherlands
F. Lebrun
Affiliation:
Service d'Astrophysique, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
N. Lund
Affiliation:
DSRI, Juliane Maries Vej 30, 2100 Copenhagen OE, Denmark
G. G. C. Palumbo
Affiliation:
Dip. di Astronomia, Universita degli Studi di Bologna, via Ranzani 1, 40127 Bologna, Italy
J. Paul
Affiliation:
Service d'Astrophysique, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
J.-P. Roques
Affiliation:
CESR, Boite Postale 4346, 31029 Toulouse, France
R. Sunyaev
Affiliation:
Space Research Institute, Profsoyuznaya 84/32, 117810 Moscow, Russia Max-Planck Institut fr Astrophysik, Postfach 1317, 85741 Garching, Germany
B. Teegarden
Affiliation:
NASA-GSFC, Code 661, Greenbelt, MD 20771, USA
P. Ubertini
Affiliation:
IASF/CNR, via del Fosso del Cavaliere, 00133 Rome, Italy
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Abstract

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The ESA observatory INTEGRAL (International Gamma-Ray Astrophysics Laboratory) is dedicated to fine imaging and spectroscopy in the energy range 15 keV to 10 Mev with concurrent X-ray (3-35 keV) and optical monitoring. It was launched on October 17, 2002 and has been succesfully operating ever since. Its two main instruments the spectrometer SPI – optimized for high resolution spectroscopy – and the imager IBIS – optimized for for high resolution imaging – are complemented by the X-ray monitor JEM-X and the optical monitor OMC. All the high energy instruments use coded mask techniques, allowing imaging in the gamma-ray range and combining wide fields of view with high spatial resolution. The presentation gives an overview of the unique properties of INTEGRAL.

Keywords

gamma rays: observationsX-rays: stars
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 1 , Symposium S230: Populations of High Energy Sources in Galaxies , August 2005 , pp. 59 - 65
Copyright
2006 International Astronomical Union