A dataset provided by the European Space Agency

Name: ESTABLISHING THE QUASAR MODE FEEDBACK WITH NUSTAR AND XMM-NEWTON
Published: 2017-09-27T22:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	079058
Title	ESTABLISHING THE QUASAR MODE FEEDBACK WITH NUSTAR AND XMM-NEWTON
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0790580101
DOI	https://doi.org/10.5270/esa-n5iidqc
Principal Investigator, PI	Dr Francesco Tombesi
Abstract	Recent Herschel observations have identified powerful large-scale molecularoutflows in ultraluminous infrared galaxies, indicating that AGN feedback canindeed influence star formation and galaxy evolution. Theoretical modelsdescribing the formation of such large-scale outflows require a putative innerAGN accretion disk wind. We found the first evidence of such a wind inIRASF11119+3257, in the form of blue-shifted Fe XXV/XXVI absorption lines withvelocity 0.25c. However, just one object does not allow to establish thevalidity of such mechanism. Here, we request simultaneous 150ks NuSTAR and 90ksXMM-Newton observations of the next most promising ULIRG, IRASF05189-2524, tocharacterize its disk wind and conclusively establish the mechanism of quasar mode feedback.
Publications	Discovery of an X-Ray Quasar Wind Driving the Cold Gas Outflow in the Ultraluminous Infrared Galaxy IRAS F05189-2524 \|Smith Robyn N. Tombesi Francesco et al. \| ApJ \| 887-69 \| 2019 \| 2019ApJ...887...69S \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...887...69S 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 Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT \|Yamada Satoshi Ueda Yoshihiro et al. \| ApJS \| 257-61 \| 2021 \| 2021ApJS..257...61Y \| http://ui.adsabs.harvard.edu/#abs/2021ApJS..257...61Y 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-09-06T15:58:46Z/2016-09-07T19:27:59Z
Version	21.51_20241115_1113
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	2017-09-27T22:00:00Z
Last Update	2026-07-09
Keywords	"ultraluminous infrared galaxy", "promising ulirg", "irasf05189 2524", "XMM-Newton", "galaxy evolution", "disk wind", "agn feedback", "NuSTAR", "XMM", "quasar mode feedback", "scale outflows require", "xxvi absorption lines", "models describing", "xmm newton", "scale molecular outflows"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Francesco Tombesi, 2017, 'ESTABLISHING THE QUASAR MODE FEEDBACK WITH NUSTAR AND XMM-NEWTON', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-n5iidqc
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.