  A simultaneous broadband analysis of X-ray data obtained with XMM-Newton and
NuSTAR observatories for the asynchronous polar source CD Ind is presented. The
spin folded lightcurve in soft 0.3-3.0 keV band shows single broad hump-like
structure superimposed with occasional narrow dips, indicating a single-pole
accretion model with a complex intrinsic absorber. Lack of strong modulation in
folded lightcurve above 3 keV reveals that emission from corresponding zone of
post-shock region (PSR) remains in view throughout the spin phase. The
broadband spectrum is modelled with a three-component absorbed plasma emission
model and absorbed isobaric cooling flow model, both of which fit the data well
with similar statistical significance. Presence of partial covering absorber is
evident in the spectra with equivalent column density
$\sim7\times10^{22}\;\text{cm}^{-2}$ and a covering fraction of $\sim 25\%$.
Strong ionised oxygen K$_{\alpha}$ line emission is detected in the spectra. We
notice spectral variability during spin phase 0.75-1.05, when there is a
considerable increase in column density of overall absorber (from $\sim 1
\times 10^{20}\;\text{cm}^{-2}$ to $\sim 9 \times 10^{20}\;\text{cm}^{-2}$). We
required at least three plasma temperatures to describe the multi-temperature
nature of the PSR. The shock temperature $\sim 43.3_{-3.4}^{+3.8}$ keV,
represented by the upper temperature of the cooling flow model, implies a white
dwarf mass of $\sim 0.87^{+0.04}_{-0.03}\;M_{\odot}$. The iron K$_{\alpha}$
line complex shows a strong He-like and a weak neutral fluorescence line. We
could not unambiguously detect the presence of Compton reflection in the
spectra, which is probably very small and signifying a tall shock height.
