activity
20122025
most citedA possible mechanism for multiple changing look phenomenon in Active Galactic Nuclei

135 citations · 596 across the 24 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

astro-ph.GA2018★ 2 cited

Fe II velocity shifts in optical spectra of type 1 AGN

E. Bon, P. Marziani, M. Berton +4

Here we present a critical view of practical problems in the analysis of optical Fe II emission lines of Type 1 AGN spectra. Besides the very complex and unclear physical interpret…

astro-ph.GA2018★ 60 cited

Highly accreting quasars: The SDSS low-redshift catalog

C. A. Negrete, D. Dultzin, P. Marziani +8

The most highly accreting quasars (xA) are of special interest in studies of the physics of AGNs and host galaxy evolution. Quasars accreting at high rates (L/LEdd 1) hold p…

astro-ph.GA2018

Narrow-line Seyfert 1s: what is wrong in a name?

P. Marziani, A. del Olmo, M. D' Onofrio +6

Narrow-line Seyfert 1s (NLSy1s) are an ill-defined class. Work done over the past 20 years as well as recent analyses show a continuity in properties (e.g., Balmer line profiles, b…

astro-ph.GA2018★ 6 cited

Exploring possible relations between optical variability time scales and broad emission line shapes in AGN

E. Bon, P. Jovanovic, P. Marziani +2

Here we investigate the connection of broad emission line shapes and continuum light curve variability time scales of type-1 Active Galactic Nuclei (AGN). We developed a new model…

astro-ph.GA2018

Spectroscopy and spectropolarimetry of AGN: from observations to modelling

L. C. Popovic, D. Ilic, E. Bon +10

Active galactic nuclei (AGN) are one of the most luminous objects in the Universe, emitting powerful continuum and line emission across all wavelength bands. They represent an impo…

astro-ph.GA2018

A main sequence for quasars

P. Marziani, D. Dultzin, J. W. Sulentic +7

The last 25 years saw a major step forward in the analysis of optical and UV spectroscopic data of large quasar samples. Multivariate statistical approaches have led to the definit…

astro-ph.GA2018★ 19 cited

AGN Broad Line Region variability in the context of Eigenvector 1: case of NGC 5548

Nataša Bon, Edi Bon, Paola Marziani

Many active galactic nuclei (AGN) show strong variability of the optical continuum. Since the line flux, profile shapes and intensity ratios are changing, we analyze the variabilit…