# Evidence for Relativistic Disk Reflection in the Seyfert 1h Galaxy/ULIRG IRAS 05189-2524 Observed by NuSTAR and XMM-Newton

## TL;DR

This study analyzes X-ray spectra from NuSTAR and XMM-Newton observations of IRAS 05189-2524, revealing relativistic disk reflection features, a rapidly spinning black hole, and a compact corona close to the black hole.

## Contribution

It provides the first detailed spectral evidence for relativistic disk reflection and high black hole spin in IRAS 05189-2524 using broadband X-ray data.

## Key findings

- Detection of a broad Fe Kα emission line extending down to 3 keV
- High reflection fraction indicating a compact corona near the black hole
- Rapid black hole spin suggested but not tightly constrained

## Abstract

We present a spectral analysis of the NuSTAR and XMM-Newton observations of the Seyfert 1h galaxy/ULIRG IRAS 05189-2524 taken in 2013. We find evidence for relativistic disk reflection in the broadband X-ray spectrum: a highly asymmetric broad Fe K$\alpha$ emission line extending down to 3 keV and a Compton scattering component above 10 keV. Physical modeling with a self-consistent disk reflection model suggests the accretion disk is viewed at an intermediate angle with a super-solar iron abundance, and a mild constraint can be put on the high-energy cutoff of the power-law continuum. We test the disk reflection modeling under different absorption scenarios. A rapid black hole (BH) spin is favored, however we cannot place a model-independent tight constraint on the value. The high reflection fraction ($R_{\rm ref} \simeq$ 2.0-3.2) suggests the coronal illuminating source is compact and close to the BH (lying within 8.7 $R_{\rm g}$ above the central BH), where light-bending effects are important.