# Multi-epoch analysis of the X-ray spectrum of the active galactic nucleus in NGC 5506

## TL;DR

This study performs a comprehensive multi-epoch X-ray spectral analysis of NGC 5506, revealing a high black hole spin and insights into the accretion disk's geometry changes over time.

## Contribution

First simultaneous multi-instrument analysis of NGC 5506's X-ray spectra over 14 years, constraining black hole spin and accretion disk properties.

## Key findings

- Black hole spin constrained to 0.93±0.04.
- Spectrum variability linked to accretion disk geometry.
- Constant soft excess component over time.

## Abstract

We present a multi-epoch X-ray spectroscopy analysis of the nearby narrow-line Seyfert I galaxy NGC 5506. For the first time, spectra taken by Chandra, XMM-Newton, Suzaku, and NuSTAR - covering the 2000-2014 time span - are analyzed simultaneously, using state-of-the-art models to describe reprocessing of the primary continuum by optical thick matter in the AGN environment. The main goal of our study is determining the spin of the supermassive black hole (SMBH). The nuclear X-ray spectrum is photoelectrically absorbed by matter with column density $\simeq 3 \times 10^{22}$ cm$^{-2}$. A soft excess is present at energies lower than the photoelectric cut-off. Both photo-ionized and collisionally ionized components are required to fit it. This component is constant over the time-scales probed by our data. The spectrum at energies higher than 2 keV is variable. We propose that its evolution could be driven by flux-dependent changes in the geometry of the innermost regions of the accretion disk. The black hole spin in NGC 5506 is constrained to be 0.93$\pm _{ 0.04 }^{0.04}$ at 90% confidence level for one interesting parameter.