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 ultra-fast outflows(UFOs) in Quasars of typical L* luminosities (logLvirgul45-46 erg/s); 2) assess therelation of UFOs and ionised outflows observed at host-galaxy scales; 3)investigate the relation between UFOs and the warmer-ionised and cold gas phasesobserved at soft X-ray energies.
Publications
The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview |Botteon, A., Shimwell, T. W., et al. | A&A | 660-78 | 2022 | 2022A&A...660A..78B | http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B
Supermassive Black Hole Winds in X-rays: SUBWAYS. I. Ultra-fast outflows in quasars beyond the local Universe |Matzeu, G. A., Brusa, M., et al. | A&A | 670-182 | 2023 | 2023A&A...670A.182M | http://ui.adsabs.harvard.edu/#abs/2023A&A...670A.182M
The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium |Zhang, X., Simionescu, A., et al. | A&A | 672-42 | 2023 | 2023A&A...672A..42Z | http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z
The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models |Cassano, R., Cuciti, V., et al. | A&A | 672-43 | 2023 | 2023A&A...672A..43C | http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C
The Hot Circumgalactic Medium of the Milky Way: New Insights from XMM-Newton Observations |Bhattacharyya, Joy, Das, Sanskriti, et al. | ApJ | 952-41 | 2023 | 2023ApJ...952...41B | http://ui.adsabs.harvard.edu/#abs/2023ApJ...952...41B
BASS-XL: X-ray variability properties of unobscured active galactic nuclei |Tortosa, Alessia, Ricci, Claudio, et al. | MNRAS | 526-1687 | 2023 | 2023MNRAS.526.1687T | http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.1687T
The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII, O VIII, and Fe L-shell Transitions |Pan, Zeyang, Qu, Zhijie, et al. | ApJS | 271-62 | 2024 | 2024ApJS..271...62P | http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P
The European Space Agencys (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESAs second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations. Since Earths atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
European Space Agency, Dr Marcella Brusa, 2021, 'Shedding X-ray light on Supermassive Black Hole winds openParSUBWAYSclosePar', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-gnaa4dc
