Shedding X-ray light on Supermassive Black Hole winds openParSUBWAYSclosePar

The proposed program is designed to provide a unique observational framework totest the validity of physical models for Active Galactic Nuclei (AGN) outflows,and to ultimately understand their impact into their host galaxies. Theimmediate goals of this 1.68 Ms large program are to 1) obtain a statisticallysound measure of the duty cycle and physical parameters of ultrafast outflows(UFOs) in Quasars of typical L* luminosities (logLvirgul4546 erg/s); 2) assess therelation of UFOs and ionised outflows observed at hostgalaxy scales; 3)investigate the relation between UFOs and the warmerionised and cold gas phasesobserved at soft Xray energies. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]