کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
1829735 | 1526488 | 2008 | 9 صفحه PDF | دانلود رایگان |
![عکس صفحه اول مقاله: INTEGRAL high energy sky: The keV to MeV cosmic sources INTEGRAL high energy sky: The keV to MeV cosmic sources](/preview/png/1829735.png)
After almost 5 years of operation, ESA's International Gamma-Ray Astrophysics Laboratory (INTEGRAL) Space Observatory has unveiled a new soft gamma-ray sky and produced a remarkable harvest of results, ranging from identification of new high energy sources, to the discovery of dozens of variable sources to the mapping of the aluminum emission from the Galaxy Plane to the presence of electrons and positrons generating the annihilation line in the Galaxy central radian. INTEGRAL is continuing the deep observations of the Galactic Plane and of the whole sky in the soft gamma-ray range. The new IBIS gamma-ray catalogue contains more than 420 sources detected above 20 keV. We present a view of the INTEGRAL high energy sky with particular regard to sources emitting at high energy, including Active Galactic Nuclei (AGN), High Energy Steroscopic System (HESS)/MAGIC counterparts and new view of the cosmic gamma-ray diffuse background.
Journal: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment - Volume 588, Issues 1–2, 1 April 2008, Pages 63–71