Title:Integral Field Spectroscopy SINFONI observation of AGN at z~1.6

Abstract:
The aim of the study is to obtain properties of distant low luminosity active 
galactic nuclei (AGN). In terms of galaxy evolution, nuclear activity seems to 
play an important role.  AGN feedback processes may have impacts on the 
predictions for galaxy properties, as these processes are thought to affect the 
efficiency of star formation. Therefore it becomes interesting to study the AGN 
host galaxy.  SINFONI is an adaptive optics assisted near infrared integral 
field spectrometer mounted to the ESO VLT.  The integral field spectroscopy 
allows us to explore spatially extended sources,  to resolve properties of high 
redshift galaxies. We present the observation of two low luminosity AGNs from 
which we want to disentangle the properties of it’s host galaxy.  The 
selected galaxies to be studied were observed with SINFONI from VLT at H band.  
A first data set reduction was perform using the ESO-SINFONI pipeline, 
additionally was used some Python routines in order to improve some reduction 
steps.  As a result we obtain the data-cube and the spectrum from which can be 
clearly observed the Ha broad emission line. The deconvolution in the AGN and 
host galaxy components is the next step in this study.