A <i>NuSTAR</i> and <i>Swift</i> view of the hard state of MAXI J1813−095

We present an analysis of the NuSTAR and Swift spectra black hole candidate MAXI J1813-095 in a failed-transition outburst 2018. The observations show evidence reflected emission from inner region accretion disc. By modelling reflection component spectra, we find disc radius $R_{\rm in}<7$ $r_{\rm g}$. This result suggests that either slightly truncated or non-truncated forms at few percent Eddington limit J1813-095. Our best-fit models indicate geometry innermost remains consistent during period observations. spectral variability multi-epoch is dominated by variable photon index Comptonisation emission.