English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

The SINFONI survey for Unveiling the Physics and Effect of Radiative feedback(SUPER) aims at tracing and characterizing ionized gas outflows and theirimpact on star formation in a statistical sample of X-ray selected ActiveGalactic Nuclei (AGN) at z$\sim$2. We present the first SINFONI results for asample of 21 Type-1 AGN spanning a wide range in bolometric luminosity (log$\mathrm{L_{bol}}$ = 45.4-47.9 erg/s). The main aims of this paper aredetermining the extension of the ionized gas, characterizing the occurrence ofAGN-driven outflows, and linking the properties of such outflows with those ofthe AGN. We use Adaptive Optics-assisted SINFONI observations to trace ionizedgas in the extended narrow line region using the [OIII]5007 line. We classify atarget as hosting an outflow if its non-parametric velocity of the [OIII] line,$\mathrm{w_{80}}$, is larger than 600 km/s. We study the presence of extendedemission using dedicated point-spread function (PSF) observations, aftermodelling the PSF from the Balmer lines originating from the Broad Line Region.We detect outflows in all the Type-1 AGN sample based on the $\mathrm{w_{80}}$value from the integrated spectrum, which is in the range 650-2700 km/s. Thereis a clear positive correlation between $\mathrm{w_{80}}$ and the AGNbolometric luminosity (99% correlation probability), but a weaker correlationwith the black hole mass (80% correlation probability). A comparison of the PSFand the [OIII] radial profile shows that the [OIII] emission is spatiallyresolved for $\sim$35% of the Type-1 sample and the outflows show an extensionup to $\sim$6 kpc. The relation between maximum velocity and the bolometricluminosity is consistent with model predictions for shocks from an AGN drivenoutflow. The escape fraction of the outflowing gas increase with the AGNluminosity, although for most galaxies, this fraction is less than 10%.

SUPER-II: Spatially resolved ionized gas kinematics and scaling relations in z~2 AGN host galaxies