Active galactic nuclei (AGNs) can be divided into two major classes, namely radio-loud and
radio-quiet AGNs. A small subset of the radio-loud AGNs is called blazars, which are …

In this paper, we use the distributions of two-component radio emissions to investigate the
consequences of relativistic beaming on the unified scheme of blazar populations and radio …

In this paper, we review the predictions of the popular relativistic beaming model for the
unification of radio-and X-ray selected BL Lac (RBL and XBL) populations. Using results of …

We study the distributions of γ γ-ray properties of a sample of γ γ-ray loud blazars taken from
the third catalogue of blazars detected by Fermi-Large Area Telescope (Fermi-LAT). We …

We utilize the distributions of fractional separation difference (x) as asymmetry parameter,
linear size (D) and core-to lobe luminosity ratio (R) as orientation indicators, to investigate a …

Our understanding of the unification of jetted active galactic nuclei (AGNs) has advanced
greatly as the size of extragalactic sources increased. In this paper, based on the large …

This paper investigates a simple consequence of relativistic beaming and radio source
orientation scenario for high-luminosity extragalactic radio sources, based on the …

Statistical analyses are invaluable methods used to understand intrinsic emission processes
and the unification of extragalactic radio sources. In this paper, we collected radio, X‐ray …

In this work, a theoretical model is developed for explanation of temporal evolution of
extragalactic radio sources via beaming, orientation effects and asymmetries. Equation of …

In this paper we use the correlation between radio core-dominance (R) and Linear size (D)
properties of a sample of AGN (ESSs and FSRQs) to investigate the beaming hypothesis …