Abstract
In this paper, we compiled 572 blazars that have known core dominance parameter (log R), out of which 121 blazars are γ-ray loud blazars. We compared log R between 121 blazars and the rest with non γ-ray detections, and found that γ-ray loud blazars showed a different distribution, and their average value of log R is greater than that for non γ-ray blazars. Our analysis suggests that the γ-ray emissions are strongly beamed.
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