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AIP Conference Proceedings, 1997
Roughly 60 blazars have been identified with >100 MeV EGRET γ-ray sources, and show inferred isotropic luminosities as large as 3×1049 ergs s−1. The two most remarkable characteristics about the EGRET observations are that the γ-ray luminosity often dominates the bolometric power, and that variability on time-scales of one day or less is seen from ...
R. C. Hartman +3 more
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Roughly 60 blazars have been identified with >100 MeV EGRET γ-ray sources, and show inferred isotropic luminosities as large as 3×1049 ergs s−1. The two most remarkable characteristics about the EGRET observations are that the γ-ray luminosity often dominates the bolometric power, and that variability on time-scales of one day or less is seen from ...
R. C. Hartman +3 more
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2014
Un gruppo di ricerca di astrofisica italiano ha recentemente confermato una scoperta intrigante riguardo ad uno dei più noti e studiati blazar: l’oggetto denominato PKS2155-304. Tramite osservazioni ottenute con il telescopio INAF REM ed osservazioni ad alta energia ottenute con il satellite NASA Fermi, si è determinata l’esistenza di una periodicità ...
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Un gruppo di ricerca di astrofisica italiano ha recentemente confermato una scoperta intrigante riguardo ad uno dei più noti e studiati blazar: l’oggetto denominato PKS2155-304. Tramite osservazioni ottenute con il telescopio INAF REM ed osservazioni ad alta energia ottenute con il satellite NASA Fermi, si è determinata l’esistenza di una periodicità ...
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Observing blazars with the Whole Earth Blazar Telescope
2002Not ...
VILLATA M +55 more
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2009
Blazars are active galactic nuclei characterized by strong, nearly pure non-thermal radiations; these extend across the electromagnetic spectrum, from radio frequencies to the most energetics γ rays observed, in some cases up to TeV energies.
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Blazars are active galactic nuclei characterized by strong, nearly pure non-thermal radiations; these extend across the electromagnetic spectrum, from radio frequencies to the most energetics γ rays observed, in some cases up to TeV energies.
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SCIENTIA SINICA Physica, Mechanica & Astronomica, 2015
JianCheng WANG, MaiChang LEI
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JianCheng WANG, MaiChang LEI
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