A dataset provided by the European Space Agency

Name: XMM-Newton observations of galaxy-wide outflows: the origin of super winds
Published: 2017-11-29T23:00:00Z

Proposal ID	078406
Title	XMM-Newton observations of galaxy-wide outflows: the origin of super winds
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784060801
DOI	https://doi.org/10.5270/esa-6vdwmnk
Principal Investigator, PI	Dr Marcella Brusa
Abstract	We propose a large program with XMM-Newton to observe, for the first time in asystematic way, a well defined sample of z~0.1-0.2 Seyfert 2 AGN withunambiguous evidence of kpc-scale outflows in the ionised gas. With the proposedobservations we will be able to characterize the targets in terms of theirnuclear parameters, and in particular distinguish between Compton Thick AGN (asexpected in the heavily obscured phase when the wind has been just launched) andunobscured/mildly obscured AGN. We will also study the relation between thenuclear properties (e.g. the Eddington rate and the presence of sub-pc scalesoutflows) and the kinetic power of the outflowing wind. Overall, the XMM-Newtondata will provide an important set of observational constraints to directly test AGN feedback models.
Publications	Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z 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 From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R Robust constraints on feebly interacting particles using XMM-Newton \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-L101305 \| 2024 \| 2024PhRvD.109j1305L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j1305L Multimessenger search for electrophilic feebly interacting particles from supernovae \|Luque Pedro De la Torre Balaji Shyam \| PhRvD \| 109-103028 \| 2024 \| 2024PhRvD.109j3028L \| http://ui.adsabs.harvard.edu/#abs/2024PhRvD.109j3028L Importance of Cosmic-Ray Propagation on Sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 968-46 \| 2024 \| 2024ApJ...968...46D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...968...46D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-11-16T04:41:04Z/2016-11-16T13:41:04Z
Version	17.56_20190403_1200
Mission Description	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.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2017-11-29T23:00:00Z
Last Update	2025-01-27
Keywords	"galaxy wide outflows", "defined sample", "eddington rate", "mildly obscured agn", "compton thick agn", "unambiguous evidence", "xmm newton", "outflowing wind", "XMM-Newton", "xmm newton data", "scale outflows", "nuclear properties", "XMM", "kinetic power", "ionised gas", "nuclear parameters", "super winds", "heavily obscured phase"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marcella Brusa, 2017, 'XMM-Newton observations of galaxy-wide outflows: the origin of super winds', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6vdwmnk