activity
20072019
most citedCIV 1549 as an Eigenvector 1 Parameter for Active Galactic Nuclei

237 citations · 351 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA201940 cited

Black hole mass estimates in quasars - A comparative analysis of high- and low-ionization lines

P. Marziani, A. del Olmo, M. A. Martinez-Carballo +7

The inter-line comparison between high- and low-ionization emission lines has yielded a wealth of information on the quasar broad line region (BLR) structure and dynamics, includin…

astro-ph.GA20187 cited

HE0359-3959: an extremely radiating quasar

M. L. Martínez-Aldama, A. Del Olmo, P. Marziani +3

We present a multiwavelength spectral study of the quasar HE0359-3959, which has been identified as an extreme radiating source at intermediate redshift (z=1.5209). Along the spect…

astro-ph.GA20174 cited

A possible binary AGN in Mrk\,622?

E. Benítez, J. M. Rodríguez-Espinosa, I. Cruz-González +5

Mrk\,622 is a Compton Thick AGN and a double-peaked narrow emission line galaxy, thus a dual AGN candidate. In this work, new optical long-slit spectroscopic observations clearly s…

astro-ph.GA2017

Quasar massive ionized outflows traced by CIV λ1549 and [OIII]λλ4959,5007

P. Marziani, C. A. Negrete, D. Dultzin +4

The most luminous quasars (with bolometric luminosities are 1E47 erg/s) show a high prevalence of CIV λ1549 and [OIII]λλ4959,5007 emission line profiles with strong blueshifts. Blu…

astro-ph.GA201763 cited

What does Civλ1549 tell us about the physical driver of the Eigenvector Quasar Sequence?

J. W. Sulentic, A. del Olmo, P. Marziani +8

Broad emission lines in quasars enable us to "resolve" structure and kinematics of the broad line emitting region (BLR) thought to in- volve an accretion disk feeding a supermassiv…

astro-ph2007237 cited

CIV 1549 as an Eigenvector 1 Parameter for Active Galactic Nuclei

Jack W. Sulentic, Rumen Bachev, Paola Marziani +2

[Abridged] We have been exploring a spectroscopic unification for all known types of broad line emitting AGN. The 4D Eigenvector 1 (4DE1) parameter space shows promise as a unifica…