Understanding AGN-host connection in partially obscured active galactic nuclei. Part III: Properties of ROSAT-selected SDSS AGNs

TL;DR

This study investigates the properties of ROSAT-selected Seyfert galaxies and composite AGNs, revealing correlations between emission line ratios and stellar population age indicators, and exploring their X-ray spectral characteristics to understand AGN-host coevolution.

Contribution

It extends previous AGN-host studies by analyzing ROSAT-selected Seyfert galaxies, establishing new correlations between line ratios and stellar age indicators, and examining X-ray spectral influences.

Findings

Strong correlation between [OI]/Hα and D_n(4000)

New correlation between [SII]/Hα and D_n(4000)

X-ray spectral slope influences emission line ratios

Abstract

As the third paper of our serial studies that are aim at examining the AGN-host coevolution by using partially obscured AGNs, we extend the broad-line composite galaxies (composite AGNs) into ROSAT-selected Seyfert 1.8/1.9 galaxies basing upon the RASS/SDSS-DR5 catalog given by Anderson et al.. The SDSS spectra of in total 92 objects are analyzed by the same method used in our previous studies, after requiring the signal-to-noise ratio in the SDSS r' band is larger than 20. Combing the ROSAT-selected Seyfert galaxies with the composite AGNs reinforces the tight correlation between the line ratio [OI]/H\alpha vs. D_n(4000), and establishes a new tight correlation between [SII]/H\alpha vs. D_n(4000). Both correlations suggest the two line ratios are plausible age indicators of the circumnuclear stellar population for typical type I AGNs in which the stellar populations are difficult to be derived from their optical spectra. The ROSAT-selected Seyfert galaxies show that the two correlations depend on the soft X-ray spectral slope \alpha_X that is roughly estimated from the hardness ratios by requiring the X-ray count rates within 0.1-2.4 keV are larger than 0.02 counts s^-1. However, we fail to establish a relationship between \alpha_X and D_n(4000), which is likely caused by the relatively large uncertainties of both parameters (especially for \alpha_X because of the AGN intrinsic obscuration). The previously established L/L_Edd-D_n(4000) evolutionary sequence is reinforced again by the extension to the ROSAT-selected Seyfert galaxies. These X-ray-selected Seyfert galaxies are, however, biased against the two ends of the sequence, which implies that the X-ray Seyfert galaxies present a population at middle evolutionary stage.