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dc.rights.license© ESO 2020-
dc.contributor.authorKakkad, D.-
dc.contributor.authorMainieri, V.-
dc.contributor.authorVietri, G.-
dc.contributor.authorCarniani, S.-
dc.contributor.authorHarrison, C. M.-
dc.contributor.authorPerna, M.-
dc.contributor.authorScholtz, J.-
dc.contributor.authorCircosta, C.-
dc.contributor.authorCresci, G.-
dc.contributor.authorHusemann, B.-
dc.contributor.authorBischetti, M.-
dc.contributor.authorFeruglio, C.-
dc.contributor.authorFiore, F.-
dc.contributor.authorMarconi, A.-
dc.contributor.authorPadovani, P.-
dc.contributor.authorBrusa, M.-
dc.contributor.authorCicone, C.-
dc.contributor.authorComastri, A.-
dc.contributor.authorLanzuisi, G.-
dc.contributor.authorMannucci, F.-
dc.contributor.authorMenci, N.-
dc.contributor.authorNetzer, H.-
dc.contributor.authorPiconcelli, E.-
dc.contributor.authorPuglisi, A.-
dc.contributor.authorSalvato, M.-
dc.contributor.authorSchramm, M.-
dc.contributor.authorSilverman, J.-
dc.contributor.authorVignali, C.-
dc.contributor.authorZamorani, G.-
dc.contributor.authorZappacosta, L.-
dc.contributor.otherUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737-
dc.date.accessioned2021-04-19T08:02:23Z-
dc.date.available2021-04-19T08:02:23Z-
dc.date.issued2020-10-13-
dc.identifier.citationAstronomy and Astrophysics 642: A147(2020)es
dc.identifier.issn0004-6361-
dc.identifier.otherhttps://www.aanda.org/articles/aa/abs/2020/10/aa38551-20/aa38551-20.html-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/402-
dc.description.abstractAims. 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 Lbol = 45.4–47.9 erg s−1). 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. 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, w80, was larger than 600 km s−1. 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. Results. We detect outflows in all the Type 1 AGN sample based on the w80 value from the integrated spectrum, which is in the range ∼650–2700 km s−1. There is a clear positive correlation between w80 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%.es
dc.description.sponsorshipWe thank the referee for the useful and constructive comments. We thank Michele Cirasuolo, Alice Concas and Dominika Wylezalek for providing the comparison data for the w<INF>80</INF> distribution. M. P. is supported by the Programa Atraccion de Talento de la Comunidad de Madrid via grant 2018-T2/TIC-11715. Based on observations collected at the European organisation for Astronomical Research in the Southern Hemisphere under ESO program 196.A-0377; With funding from the Spanish government through the "María de Maeztu Unit of Excellence" accreditation (MDM-2017-0737).es
dc.language.isoenges
dc.publisherEDP Scienceses
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectGalaxies: Activees
dc.subjectGalaxies: evolutiones
dc.subjectGalaxies: high redshiftes
dc.subjectTechniques: imaging spectroscopyes
dc.subjectQuarsars: emission lineses
dc.titleSUPER II. Spatially resolved ionised gas kinematics and scaling relations in z  ∼  2 AGN host galaxieses
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidKakkad, D. [0000-0002-2603-2639]-
dc.contributor.orcidManieri, V. [0000-0002-1047-9583]-
dc.contributor.orcidVietri, G. [0000-0001-9155-8875]-
dc.contributor.orcidCarniani, S. [0000-0002-6719-380X]-
dc.contributor.orcidPerna, M. [0000-0002-0362-5941]-
dc.contributor.orcidCreci, G. [0000-0002-5281-1417]-
dc.contributor.orcidHusemann, B. [0000-0003-2901-6842]-
dc.contributor.orcidBischetti, M. [0000-0002-4314-021X]-
dc.contributor.orcidFiore, F. [0000-0002-4031-4157]-
dc.contributor.orcidMarconi, A. [0000-0002-9889-4238]-
dc.contributor.orcidPadovani, P. [0000-0002-4707-6841]-
dc.contributor.orcidCicone, C. [0000-0003-0522-6941]-
dc.contributor.orcidComastri, A. [0000-0003-3451-9970]-
dc.contributor.orcidMannucci, F. [0000-0002-4803-2381]-
dc.identifier.doi10.1051/0004-6361/202038551-
dc.identifier.e-issn1432-0746-
dc.contributor.funderComunidad de Madrid-
dc.description.peerreviewedPeer reviewes
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
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