089107

In the highly polarised NLS1 Mrk1239 comma the primary X-ray emission from the inner black hole region appears to be completely absorbed revealing the underlying host galaxy emission. This low energy emission-line spectrum was fitted with a combination of a collisionally ionised plasma and cold comma optically thick reflected emission from the distant torus. With the highest sensitivity NuSTAR spectra comma we will peer through the absorbing column to accurately determine the continuum model comma the level of absorption comma and the distant torus parameters. Constraining the torus parameters will allow us to utilize simultaneous XMM RGS data to determine the origin of the photoionised emission at low energies.