activity
20152017
most citedMulti-color optical monitoring of the quasar 3C 273 from 2005 to 2016

58 citations · 165 across the 8 of their papers we have counts for

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Showing 2015Show all

6 papers · 1 filter

astro-ph.HE2015★ 27 cited

Multi-color optical monitoring of Mrk 501 from 2010 to 2015

Dingrong Xiong, Xiong Zhang, Tingfeng Yi +5

We have monitored the BL Lac object Mrk 501 in optical , and bands from 2010 to 2015. For Mrk 501, the presence of strong host galaxy component can affect the results of…

astro-ph.HE2015

From the "blazar sequence" to unification of blazars and radio galaxies

Dingrong Xiong, Xiong Zhang, Jinming Bai +1

Based on a large Fermi blazar sample, the blazar sequence (synchrotron peak frequency versus synchrotron peak luminosity ) is revisited. It is found th…

astro-ph.HE2015★ 12 cited

Jet/accretion and Unification for FSRQs/FRII and BL Lac objects/FRI radio galaxies

Yongyun Chen, Xiong Zhang, Haojing Zhang +5

We compiled a sample of 24 flat-spectrum radio quasars (FSRQs), 21 BL Lacs, 13 FRI and 12 FRII radio galaxies to study the jet power and broad-line luminosity relation, and the jet…

astro-ph.HE2015★ 12 cited

The jets-accretion relation, mass-luminosity relation in Fermi blazars

Xiaoling Yu, Xiong Zhang, Haojing Zhang +6

A sample of 111 Fermi blazars each with a well-established radio core luminosity, broad-line luminosity, bolometric luminosity and black hole mass has been compiled from the litera…

astro-ph.HE2015★ 33 cited

Basic properties of Fermi blazars and the "blazar sequence"

Dingrong Xiong, Xiong Zhang, Jinming Bai +1

By statistically analyzing a large sample which includes blazars of Fermi detection (FBs) and non-Fermi detection (NFBs), we find that there are significant differences between FBs…

astro-ph.HE2015★ 1 cited

Core-dominance parameter, black hole mass and jet-disc connection in Fermi blazars

Y. Y. Chen, X. Zhang, H. J. Zhang +1

We study the relationship between jet power and accretion for Fermi and non-Fermi blazars, respectively. We also compare the relevant parameter between them. Our main results are a…