The variations of very-high energy γ-quanta flux from the blazar 3C 66A in 2002
Vernadsky National Library of Ukraine
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Title |
The variations of very-high energy γ-quanta flux from the blazar 3C 66A in 2002
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Creator |
Fidelis, V.V.
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Subject |
MS3: Physics of Stars and Galaxies
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Description |
The extra-galactic source blazar 3C 66A was observed in 2002 with the aid of the air Cherenkov telescope GT-48 dedicated for stereoscopic measurements of extensive air showers (EAS). The analysis of the observational data obtained during the period November–December with a total exposure time of 6h40m revealed a γ-ray flux atE >1 TeV ≈ 93% of the steady flux from the Crab Nebula at 5.03 σ level. The observations have shown variations of flux intensity from source in the very-high energy (VHE) band which may be interpreted as low and high states of the object during the observing period. The temporal properties of object are correlated well with quasi-simultaneous observations in the 2–10 keV energy band as measured by the All Sky Monitor onboard RXTE.
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Date |
2015-04-03T17:03:50Z
2015-04-03T17:03:50Z 2005 |
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Type |
Article
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Identifier |
The variations of very-high energy γ-quanta flux from the blazar 3C 66A in 2002 / V.V. Fidelis // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 205-210. — Бібліогр.: 21 назв. — англ.
0233-7665 http://dspace.nbuv.gov.ua/handle/123456789/79644 |
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Language |
en
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Relation |
Кинематика и физика небесных тел
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Publisher |
Головна астрономічна обсерваторія НАН України
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