NuSTAR view of heavily absorbed AGN: The $R-N_\text{H}$ correlation

The nature of the putative torus and the outer geometry of active galactic nuclei (AGN) are still rather unknown and the subject of active research. Improving our understanding of them is crucial for developing a physical picture for the structure of AGN. The main goal of this work is to investigate the outer geometry of AGN by studying the observed hard X-ray spectrum of obscured sources. We primarily aim at researching the reflected emission in these sources. To that end, we analysed archived NuSTAR observations of a sample of nearby AGN, whose X-ray emission has been found to be heavily absorbed, with $10^{23} 1.5\cdot 10^{24}\text{ cm}^{-2}$) regime.