A dataset provided by the European Space Agency

Name: Connecting compact ultra-fast outflows with galaxy-wide AGN-driven winds
Published: 2018-08-30T22:00:00Z

Proposal ID	080351
Title	Connecting compact ultra-fast outflows with galaxy-wide AGN-driven winds
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0803510201
DOI	https://doi.org/10.5270/esa-t2swk7u
Principal Investigator, PI	Dr Mirko Krumpe
Abstract	We propose a deep 175 ks observation of the close-by, X-ray bright AGNHE1353-1917. MUSE, a ground-breaking new IFU spectrograph on the VLT, providedunprecedented 3D coverage of the object. The optical data show the strongestevidence of a kpc-scale outflow from an AGN in a well-defined sample of luminousnearby AGN. The search for signs of X-ray outflows (ultra-fast outflows and/orwarm absorbers) will identify whether or not these (sub)parsec-scale X-rayoutflows of the AGN can be connected to the kilo-parsec optical phenomena. Usingboth X-ray and existing IFU data will enable us to connect the velocity profileas a function of distance from the center. The results will be used to constrainif the outflows are momentum- or energy-driven.
Publications	The Close AGN Reference Survey (CARS). A massive multi-phase outflow impacting the edge-on galaxy HE 1353-1917 \|Husemann B. Scharwachter J. et al. \| A&A \| 627-53 \| 2019 \| 2019A&A...627A..53H \| http://ui.adsabs.harvard.edu/#abs/2019A&A...627A..53H 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 A Systematic Study of the Short-term X-Ray Variability of Seyfert Galaxies. I. Diversity of the X-Ray rms Spectra \|Hu Jingwei Jin Chichuan et al. \| ApJ \| 936-105 \| 2022 \| 2022ApJ...936..105H \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...936..105H 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	2017-08-08T04:52:29Z/2017-08-08T22:05:49Z
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	2018-08-30T22:00:00Z
Last Update	2025-01-27
Keywords	"optical data", "deep 175", "warm absorbers", "ifu spectrograph", "ground breaking", "energy driven", "velocity profile", "strongest evidence", "3d coverage", "luminous nearby agn", "scale outflow", "defined sample", "existing ifu data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Mirko Krumpe, 2018, 'Connecting compact ultra-fast outflows with galaxy-wide AGN-driven winds', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-t2swk7u