# Spectral properties of NGC 4151 and the Estimation of black hole mass using TCAF solution

## TL;DR

This study applies the novel TCAF spectral model to X-ray data of NGC 4151, estimating the supermassive black hole mass and analyzing accretion flow properties, marking the first such application to an AGN.

## Contribution

First implementation of the TCAF model on AGN X-ray spectra to estimate black hole mass and accretion flow characteristics.

## Key findings

- Estimated black hole mass: ~3.03 x 10^7 M_sun
- Accretion flow was in a hard state during observation
- Flow geometry and accretion rates were characterized

## Abstract

We present X-ray spectral analysis of Seyfert 1.5 Active Galactic Nuclei (AGN) NGC~4151 using \textit{NuSTAR} observation during 2012. This is the first attempt to fit an AGN data using the physical Two Component Advective flow (TCAF) solution. We disentangle the continuum emission properties of the source in the energy range $3.0$ to $70.0$~keV using the spectrum obtained from TCAF model. This model was used as an additive local model directly in {\fontfamily{qcr}\selectfont XSPEC}. Additionally, we used a power law (PL) component, to take care of possible X-ray contribution from the jet, which is not incorporated in the present version of TCAF. Our primary aim is to obtain the flow properties and the mass of the central supermassive black hole from the available archival data. Our best estimate of the average mass obtained from spectral fits of three observations, is $M_{BH}=3.03^{+0.26}_{-0.26}\times 10^7 M_\odot$. This is consistent with earlier estimations in the literature such as reverberation mapping, gas kinematics and stellar dynamics around black holes. We also discuss the accretion dynamics and the flow geometry on the basis of model fitted physical parameters. Model fitted disk accretion rate is found to be lower than the low angular momentum halo accretion rate, indicating that the source was in a hard state during the observation.