# The properties of active galaxies at the extreme of eigenvector 1

## TL;DR

This study investigates the extreme properties of eigenvector 1 in unobscured type 1 active galaxies, analyzing SDSS quasars to understand the nature of EV1 and its relation to quasar spectral features.

## Contribution

The paper provides a detailed analysis of the most extreme eigenvector 1 quasars, highlighting the diversity in their spectral properties and challenging the interpretation of EV1.

## Key findings

- Only 6 out of 27 high R_Fe sources confirmed with R_Fe > 1.3
- High R_Fe objects show diverse Hβ line widths, from narrow to broad
- The interpretation of EV1 remains unresolved due to spectral diversity

## Abstract

Eigenvector 1 (EV1) is the formal parameter which allows the introduction of some order in the properties of the unobscured type 1 active galaxies. We aim to understand the nature of this parameter by analyzing the most extreme examples of quasars with the highest possible values of the corresponding eigenvalues $R_{Fe}$. We selected the appropriate sources from the Sloan Digital Sky Survey (SDSS) and performed detailed modeling, including various templates for the Fe II pseudo-continuum and the starlight contribution to the spectrum. Out of 27 sources with $R_{Fe}$ larger than 1.3 and with the measurement errors smaller than 20\% selected from the SDSS quasar catalog, only six sources were confirmed to have a high value of $R_{Fe}$, defined as being above 1.3. All other sources have $an R_{Fe}$ of approximately 1. Three of the high $R_{Fe}$ objects have a very narrow H$\beta$ line, below 2100 km s$^{-1}$ but three sources have broad lines, above 4500 km s$^{-1}$, that do not seem to form a uniform group, differing considerably in black hole mass and Eddington ratio; they simply have a very similar EW([OIII]5007) line. Therefore, the interpretation of the EV1 remains an open issue.