Kakkad, D.D.KakkadMainieri, V.V.MainieriVIETRI, GiustinaGiustinaVIETRICarniani, S.S.CarnianiHarrison, C. M.C. M.HarrisonPerna, M.M.PernaScholtz, J.J.ScholtzCircosta, C.C.CircostaCRESCI, GiovanniGiovanniCRESCIHusemann, B.B.HusemannBISCHETTI, ManuelaManuelaBISCHETTIFERUGLIO, ChiaraChiaraFERUGLIOFIORE, FabrizioFabrizioFIOREMARCONI, AlessandroAlessandroMARCONIPadovani, P.P.PadovaniBrusa, M.M.BrusaCICONE, CLAUDIACLAUDIACICONECOMASTRI, AndreaAndreaCOMASTRILANZUISI, GiorgioGiorgioLANZUISIMANNUCCI, FilippoFilippoMANNUCCIMENCI, NicolaNicolaMENCINetzer, H.H.NetzerPICONCELLI, EnricoEnricoPICONCELLIPUGLISI, Alfio TimothyAlfio TimothyPUGLISISalvato, M.M.SalvatoSchramm, M.M.SchrammSilverman, J.J.SilvermanVignali, C.C.VignaliZamorani, G.G.ZamoraniZAPPACOSTA, LucaLucaZAPPACOSTA2025-02-182025-02-1820200004-6361http://hdl.handle.net/20.500.12386/36041<BR /> Aims: The SINFONI survey for Unveiling the Physics and Effect of Radiative feedback (SUPER) aims to trace and characterise ionised gas outflows and their impact on star formation in a statistical sample of X-ray selected active galactic nuclei (AGN) at z ∼ 2. We present the first SINFONI results for a sample of 21 Type 1 AGN spanning a wide range in bolometric luminosity (log L<SUB>bol</SUB> = 45.4-47.9 erg s<SUP>-1</SUP>). The main aims of this paper are to determine the extension of the ionised gas, characterise the occurrence of AGN-driven outflows, and link the properties of such outflows with those of the AGN. <BR /> Methods: We used adaptive optics-assisted SINFONI observations to trace ionised gas in the extended narrow line region using the [O III] λ5007 line. We classified a target as hosting an outflow if its non-parametric velocity of the [O III] line, w<SUB>80</SUB>, was larger than 600 km s<SUP>-1</SUP>. We studied the presence of extended emission using dedicated point-spread function (PSF) observations, after modelling the PSF from the Balmer lines originating from the broad line region. <BR /> Results: We detect outflows in all the Type 1 AGN sample based on the w<SUB>80</SUB> value from the integrated spectrum, which is in the range ∼650-2700 km s<SUP>-1</SUP>. There is a clear positive correlation between w<SUB>80</SUB> and the AGN bolometric luminosity (> 99% correlation probability), and the black hole mass (98% correlation probability). A comparison of the PSF and the [O III] radial profile shows that the [O III] emission is spatially resolved for ∼35% of the Type 1 sample and the outflows show an extension up to ∼6 kpc. The relation between maximum velocity and the bolometric luminosity is consistent with model predictions for shocks from an AGN-driven outflow. The escape fraction of the outflowing gas increases with the AGN luminosity, although for most galaxies, this fraction is less than 10%....STAMPAenArticle10.1051/0004-6361/202038551http://arxiv.org/abs/2008.01728v1https://www.aanda.org/articles/aa/full_html/2020/10/aa38551-20/aa38551-20.htmlFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation