Estimating black hole masses in obscured AGN using X-rays

Abstract

Determining the black hole masses in active galactic nuclei (AGN) is of crucial importance to constrain the basic characteristics of their central engines and shed light on their growth and co-evolution with their host galaxies. While the black hole mass (MBH) can be robustly measured with dynamical methods in bright type 1 AGN, where the variable primary emission and the broad line region (BLR) are directly observed, a direct measurement is considerably more challenging if not impossible for the vast majority of heavily obscured type 2 AGN. In this work, we tested the validity of an X-ray-based scaling method to constrain the MBH in heavily absorbed AGN. To this end, we utilized a sample of type 2 AGN with good-quality hard X-ray data obtained by the nuSTAR satellite and with MBH dynamically constrained from megamaser measurements. Our results indicate that, when the X-ray broadband spectra are fitted with physically motivated self-consistent models that properly account for absorption, scattering, and emission line contributions from the putative torus and constrain the primary X-ray emission, then the X-ray scaling method yields MBH values that are consistent with those determined from megamaser measurements within their respective uncertainties. With this method we can therefore systematically determine the MBH in any type 2 AGN, provided that they possess good-quality X-ray data and accrete at a moderate to high rate.

15 pages, 6 figures, 5 tables, accepted for publication in MNRAS

References in corpus (15)

• X-ray Properties of Black-Hole Binaries
• Simultaneous X-ray/optical/UV snapshots of active galactic nuclei from XMM-Newton: spectral energy distributions for the reverberation mapped sample
• The Hard X-ray Spectrum as a Probe for Black-Hole Growth in Radio-Quiet Active Galactic Nuclei
• The 2-79 keV X-ray Spectrum of the Circinus Galaxy with NuSTAR, XMM-Newton and Chandra: a Fully Compton-Thick AGN
• The variable hard X-ray emission of NGC4945 as observed by NuSTAR
• Broadband Observations of the Compton-thick Nucleus of NGC 3393
• The Parsec-scale Accretion Disk in NGC 3393
• The soft X-ray excess: NLS1s vs. BLS1s
• Black hole mass determination in the X-ray binary 4U 1630--47: Scaling of spectral and variability characteristics
• Consistency of the black hole mass determination in AGN from the reverberation and the X-ray excess variance method
• A growth-rate indicator for Compton-thick active galactic nuclei
• ESO 243-49 HLX-1: scaling of X-ray spectral properties and black hole mass determination
• Constraining black hole masses in low-accreting AGN using X-ray spectra
• Water megamaser emission in hard X-ray selected AGN
• Measuring the black hole mass in Ultraluminous X-ray Sources with the X-ray Scaling Method