activity
19932023
most citedEigenvector 1: An Optimal Correlation Space for Active Galactic Nuclei

323 citations · 4.9k across the 142 of their papers we have counts for

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Showing 2016Show all

7 papers · 1 filter

astro-ph.GA2016★ 22 cited

Emission Line Galaxies and Active Galactic Nuclei in WINGS clusters

P. Marziani, M. D'Onofrio, D. Bettoni +7

We present the analysis of the emission line galaxies members of 46 low redshift (0.04 < z < 0.07) clusters observed by WINGS (WIde-field Nearby Galaxy cluster Survey, Fasano et al…

astro-ph.GA2016★ 14 cited

The Extreme Ultraviolet Variability of Quasars

Brian Punsly, Paola Marziani, Shaohua Zhang +2

We study the extreme ultraviolet (EUV) variability (rest frame wavelengths 500 - 920 ) of high luminosity quasars using HST (low to intermediate redshift sample) and SDSS (high…

astro-ph.GA2016★ 1 cited

On the origin of the Fundamental Plane and Faber-Jackson relations: consequences for the star formation problem

Mauro D'Onofrio, Stefano Cariddi, Cesare Chiosi +2

The aim of this work is to show that the origin of the Fundamental Plane (FP) relation for early-type galaxies (ETGs) can be traced back to the existence of a fine-tuning between t…

astro-ph.CO2016

Tracing dark energy with quasars

J. Średzińska, B. Czerny, M. Bilicki +7

The nature of dark energy, driving the accelerated expansion of the Universe, is one of the most important issues in modern astrophysics. In order to understand this phenomenon, we…

astro-ph.HE2016★ 83 cited

Evidence for periodicity in 43 year-long monitoring of NGC 5548

E. Bon, S. Zucker, H. Netzer +14

We present an analysis of 43 years (1972 to 2015) of spectroscopic observations of the Seyfert 1 galaxy NGC 5548. This includes 12 years of new unpublished observations (2003 to 20…

astro-ph.GA2016★ 5 cited

The Extreme Ultraviolet Spectra of Low Redshift Radio Loud Quasars

Brian Punsly, Cormac Reynolds, Paola Marziani +1

This paper reports on the extreme ultraviolet (EUV) spectrum of three low redshift () radio loud quasars, 3C 95, 3C 57 and PKS 0405-123. The spectra were obtained with…