A dataset provided by the European Space Agency

Name: Exploring the Powerful Ionised Wind in the Seyfert Galaxy PG1211+143
Published: 2015-07-17T22:00:00Z

Proposal ID	074511
Title	Exploring the Powerful Ionised Wind in the Seyfert Galaxy PG1211+143
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110701
DOI	https://doi.org/10.5270/esa-755ejfc
Principal Investigator, PI	Prof Ken Pounds
Abstract	Highly-ionised high-speed winds in AGN (UFOs) were first detected withXMM-Newton a decade ago, and are now established as a key factor in the study ofSMBH accretion, and in the growth and metal enrichment of their host galaxies.However, information on the ionisation and dynamical structure, and the ultimatefate of UFOs remains very limited. We request a 600ks extended XMM-Newton studyof the prototype UFO PG1211+143 in AO-13, to obtain high quality EPIC and RGSspectra, to map the flow structure and variability, while seeking evidence forthe anticipated interaction with the ISM and possible conversion of theenergetic wind to a momentum-driven flow.
Publications	NuSTAR Reveals Relativistic Reflection But No Ultra-Fast Outflow in the Quasar Pg~1211+143 \|Zoghbi A. Miller J. M. et al. \| ApJ \| 799-24 \| 2015 \| 2015ApJ...799L..24Z \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...799L..24Z X-ray timing analysis of the quasar PG 1211+143 \|Lobban A. P. Vaughan S. et al. \| MNRAS \| 457-38 \| 2016 \| 2016MNRAS.457...38L \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.457...38L Detection of a second high-velocity component in the highly ionized wind from PG 1211+143 \|Pounds Ken Lobban Andrew et al. \| MNRAS \| 457-2951 \| 2016 \| 2016MNRAS.457.2951P \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.457.2951P XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N A dual velocity in the highly ionized wind of the luminous narrow line Seyfert galaxy PG 1211+143 \|Pounds K. A. Lobban A. et al. \| AN \| 337-518 \| 2016 \| 2016AN....337..518P \| http://ui.adsabs.harvard.edu/#abs/2016AN....337..518P Imprints of a high-velocity wind on the soft X-ray spectrum of PG1211+143 \|Pounds K. A. Lobban A. et al. \| MNRAS \| 459-4389 \| 2016 \| 2016MNRAS.459.4389P \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.459.4389P A search for X-ray reprocessing echoes in the power spectral density functions of AGN \|Emmanoulopoulos D. Papadakis I. E. et al. \| MNRAS \| 461-1642 \| 2016 \| 2016MNRAS.461.1642E \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461.1642E The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Testing Relativistic Reflection and Resolving Outflows in PG 1211+143 with XMM-Newton and NuSTAR \|Lobban A. P. Pounds K. et al. \| ApJ \| 831-201 \| 2016 \| 2016ApJ...831..201L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...831..201L Leveraging high-resolution spectra to understand black hole spectra \|Nowak M. A. \| AN \| 338-227 \| 2017 \| 2017AN....338..227N \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..227N Exploring accretion disk physics and black hole growth with regular monitoring of ultrafast active galactic nucleus winds \|Pounds K. Lobban A. \| AN \| 338-249 \| 2017 \| 2017AN....338..249P \| http://ui.adsabs.harvard.edu/#abs/2017AN....338..249P The Variable Fast Soft X-Ray Wind in PG 1211+143 \|Reeves J. N. Lobban A. \| ApJ \| 854-28 \| 2018 \| 2018ApJ...854...28R \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...854...28R X-ray time lags in PG 1211+143 \|Lobban A. P. Vaughan S. et al. \| MNRAS \| 476-225 \| 2018 \| 2018MNRAS.476..225L \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.476..225L Are narrow-line Seyfert 1 galaxies highly accreting low-MBH AGNs? \|Williams James K. Gliozzi Mario \| MNRAS \| 480-96 \| 2018 \| 2018MNRAS.480...96W \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480...96W An ultrafast inflow in the luminous Seyfert PG1211+143 \|Pounds K. A. Nixon C. J. et al. \| MNRAS \| 481-1832 \| 2018 \| 2018MNRAS.481.1832P \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.481.1832P The soft X-ray excess: NLS1s versus BLS1s \|Gliozzi Mario Williams James K. \| MNRAS \| 491-532 \| 2020 \| 2020MNRAS.491..532G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.491..532G A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O On the Observational Difference between the Accretion Disk-Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei \|Liu Hezhen Luo B. et al. \| ApJ \| 910-103 \| 2021 \| 2021ApJ...910..103L \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910..103L 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 X-ray timing and spectral analysis of reverberating active galactic nuclei \|Hancock S. Young A. J. \| MNRAS \| 514-5403 \| 2022 \| 2022MNRAS.514.5403H \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514.5403H 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 X-ray emission of the radio-loud quasar SDSS J121426.52+140258.9: independent variations between optical/UV and X-ray emission \|Zhou Minhua Gu Minfeng et al. \| MNRAS \| 519-909 \| 2023 \| 2023MNRAS.519..909Z \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519..909Z Investigating scaling relations in X-ray reverberating AGN using symbolic regression \|Thongkonsing P. Chainakun P. et al. \| MNRAS \| 527-1950 \| 2024 \| 2024MNRAS.527.1950T \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.527.1950T 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 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 Low-redshift absorption in the Seyfert galaxy PG1211+143 - a distant inflow maintaining off-plane accretion or the gravitational redshift of matter orbiting the SMBH? \|Pounds Ken Page Kim \| MNRAS \| 531-4852 \| 2024 \| 2024MNRAS.531.4852P \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531.4852P
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2014-06-02T04:54:14Z/2014-07-09T01:42:16Z
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	2015-07-17T22:00:00Z
Last Update	2025-01-27
Keywords	"seyfert galaxy pg1211", "xmm newton", "rgs spectra", "quality epic", "smbh accretion", "decade ago", "anticipated interaction", "agn ufos", "powerful ionised wind", "speed winds", "EPIC", "XMM-Newton", "metal enrichment", "dynamical structure", "flow structure", "seeking evidence", "momentum driven flow", "prototype ufo pg1211", "energetic wind", "XMM", "key factor"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Ken Pounds, 2015, 'Exploring the Powerful Ionised Wind in the Seyfert Galaxy PG1211+143', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-755ejfc