The INTEGRAL mission

@article{Winkler1998TheIM,
  title={The INTEGRAL mission},
  author={C. Winkler and T. Courvoisier and G. Cocco and N. Gehrels and {\'A}. Gim{\'e}nez and S. Grebenev and W. Hermsen and J. Mas-Hesse and F. Lebrun and N. Lund and G. Palumbo and J. Paul and J. Roques and H. Schnopper and V. Sch{\"o}nfelder and R. Sunyaev and B. Teegarden and P. Ubertini and G. Vedrenne and A. Dean},
  journal={Astronomy and Astrophysics},
  year={1998},
  volume={411}
}
The ESA observatory INTEGRAL (International Gamma-Ray Astrophysics Laboratory) is dedicated to the fine spectroscopy (2.5 keV FWHM @ 1 MeV) and fine imaging (angular resolution: 12 arcmin FWHM) of celestial gamma-ray sources in the energy range 15 keV to 10 MeV with concurrent source monitoring in the X-ray ($3{-}35$ keV) and optical ( V -band, 550 nm) energy ranges. INTEGRAL carries two main gamma-ray instruments, the spectrometer SPI (Vedrenne et al. [CITE]) – optimized for the high… Expand
...
1
2
3
4
5
...