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Cited by 175 publications
(184 citation statements)
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References 38 publications
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“…This is in fact quite close to the maximum derived in various models in the literature, e.g., [ 26,27,28,19,163]. Therefore, should the observations conclusively demonstrate that the spectrum continues straight to above 10 TeV photon energy (for which there may be some indication), then the leptonic models would begin to have serious difficulties.…”
Section: Tev and ν-Astronomy (Rhode Bean)supporting
confidence: 85%
“…This is in fact quite close to the maximum derived in various models in the literature, e.g., [ 26,27,28,19,163]. Therefore, should the observations conclusively demonstrate that the spectrum continues straight to above 10 TeV photon energy (for which there may be some indication), then the leptonic models would begin to have serious difficulties.…”
Section: Tev and ν-Astronomy (Rhode Bean)supporting
confidence: 85%
“…This picture is consistent with the fact that the TeV emission has been observed only from the HBLs, which turned out to have higher 7 e /. For QHBs, where a dense external radiation fields exist, the ERC emission most likely contributes as much or even more significantly than the SSC emission in 7-ray band (see, e.g., Sikora et al 1997). Therefore, our analysis indicates that the difference of 7 e ; is related to the large photon density in QHBs as compared with that of HBLs; Compton upscattering of these photons may well provide the observed GeV flux.…”
Section: Multiband Analysis Of Blazarssupporting
confidence: 84%
“…The total power radiated in the γ-ray band (Sikora et al 1997) , which is almost 20 times higher than the five-year average flux. When the data are further re-binned using six-hour bins, we notice a high γ-ray flux of (9.37 ± 1.74) × 10 −7 --ph cm s 2 1…”
Section: Short-term Flux Variability and Jet Energeticsmentioning
confidence: 80%