A dataset provided by the European Space Agency

Name 074511
Title Exploring the Powerful Ionised Wind in the Seyfert Galaxy PG1211+143
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110301
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110401
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110501
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110601
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0745110701

DOI 10.5270/esa-755ejfc
Author Prof Ken Pounds
Description Highly-ionised high-speed winds in AGN (UFOs) were first detected with XMM-Newton a decade ago, and are now established as a key factor in the study of SMBH accretion, and in the growth and metal enrichment of their host galaxies. However, information on the ionisation and dynamical structure, and the ultimate fate of UFOs remains very limited. We request a 600ks extended XMM-Newton study of the prototype UFO PG1211+143 in AO-13, to obtain high quality EPIC and RGS spectra, to map the flow structure and variability, while seeking evidence for the anticipated interaction with the ISM and possible conversion of the energetic wind to a momentum-driven flow.
Publication NuSTAR Reveals Relativistic Reflection But No Ultra-Fast Outflow in the Quasar Pg~1211+143 . Zoghbi, A., Miller, J. M., et all. . ApJ . 799-24 . 2015 . 2015ApJ...799L..24Z ,
X-ray timing analysis of the quasar PG 1211+143 . Lobban, A. P., Vaughan, S., et all. . MNRAS . 457-38 . 2016 . 2016MNRAS.457...38L ,
Detection of a second high-velocity component in the highly ionized wind from PG 1211+143 . Pounds, Ken, Lobban, Andrew, et all. . MNRAS . 457-2951 . 2016 . 2016MNRAS.457.2951P ,
XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 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 all. . AN . 337-518 . 2016 . 2016AN....337..518P ,
Imprints of a high-velocity wind on the soft X-ray spectrum of PG1211+143 . Pounds, K. A., Lobban, A., et all. . MNRAS . 459-4389 . 2016 . 2016MNRAS.459.4389P ,
A search for X-ray reprocessing echoes in the power spectral density functions of AGN . Emmanoulopoulos, D., Papadakis, I. E., et all. . MNRAS . 461-1642 . 2016 . 2016MNRAS.461.1642E ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Testing Relativistic Reflection and Resolvi...
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 Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2015-07-17T22:00:00Z, 074511, 17.56_20190403_1200. https://doi.org/10.5270/esa-755ejfc