  We present the joint Chandra, XMM-Newton and NuSTAR analysis of two nearby
Seyfert galaxies, NGC 3081 and ESO 565-G019. These are the only two having
Chandra data in a larger sample of ten low redshift ($z \le 0.05$), candidates
Compton-thick Active Galactic Nuclei (AGN) selected in the 15-150 keV band with
Swift-BAT that were still lacking NuSTAR data. Our spectral analysis, performed
using physically-motivated models, provides an estimate of both the
line-of-sight (l.o.s.) and average (N$_{H,S}$) column densities of the two
torii. NGC 3081 has a Compton-thin l.o.s. column density N$_{H,z}$=[0.58-0.62]
$\times 10^{24}$cm$^{-2}$, but the N$_{H,S}$, beyond the Compton-thick
threshold (N$_{H,S}$=[1.41-1.78] $\times 10^{24}$cm$^{-2}$), suggests a
"patchy" scenario for the distribution of the circumnuclear matter. ESO
565-G019 has both Compton-thick l.o.s. and N$_{H,S}$ column densities
(N$_{H,z}>$2.31 $\times 10^{24}$cm$^{-2}$ and N$_{H,S} >$2.57 $\times
10^{24}$cm$^{-2}$, respectively). The use of physically-motivated models,
coupled with the broad energy range covered by the data (0.6-70 keV and 0.6-40
keV, for NGC 3081 and ESO 565-G019, respectively) allows us to constrain the
covering factor of the obscuring material, which is C$_{TOR}$=[0.63-0.82] for
NGC 3081, and C$_{TOR}$=[0.39-0.65] for ESO 565-G019.
