Title: INTEGRAL FIELD SPECTROSCOPY OBSERVATION of  z~1.5 AGN

Abstract:
We present the observation of two AGN with SINFONI in the H-band.  The original aim of this 
project was to observe if the host galaxies are kinematically disturbed and how this compare to 
the non-active galaxies. 
The brightest object QSO1, at $z=1.31$, has a luminosity of $L_{H\alpha} = 8.26\times10^{45}\ 
erg/s$ whereas the second object QSO2 at $z=1.55$ has a luminosity of $L_{H\alpha} = 
4.38\times10^{44}\ erg/s$. 
These QSO are at different phase of their accretion episode: QSO1 is at the peak of its quasar 
phase whereas QSO2’s SMBH is starving.
Our hypothesis is that the host galaxy contributes to the narrow-line component of the $H_
{\alpha}$ line.
In QSO1 we found a broad-component ($v>1000\ km/s$) and a narrow-component ($v>1000\ 
km/s$), however it was not possible to spatially resolve the emission of the host galaxy. 
If we assume that the total flux of the narrow component is coming from the host galaxy we 
obtain an extremely large SFR and we conclude therefore that we are observing the AGN narrow 
line region. 
Whereas for QSO2 we only observe a broad component.
With the $H_{\alpha}$ emission we estimate the  black hole mass for both objects and compare 
it to the \MgII\ based estimate.