A dataset provided by the European Space Agency

Name: The Ultrafast Outflow of the Lensed z=1.51 AGN HS 0810+2554
Published: 2015-10-29T23:00:00Z

Proposal ID	072899
Title	The Ultrafast Outflow of the Lensed z=1.51 AGN HS 0810+2554
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0728990101
DOI	https://doi.org/10.5270/esa-beclutc
Principal Investigator, PI	Dr George Chartas
Abstract	Massive and ultrafast wide-angled outflows from AGN are one of the proposedfeedback mechanisms that may provide the coupling of kinetic energy betweenquasars and their host galaxies. To further our understanding of the AGNa??srole in this process we propose joint Chandra and XMM observations of theoutflow of the z=1.5 AGN HS 0810+2554. The factor of 120 lensing magnificationof HS0810 makes this source exceptionally bright compared to other quasars withdetected outflows at similar distances. We will also study the short andlong-term variability of the X-ray outflow and the correlation of X-ray windproperties to the X-ray and UV spectral properties. The variability andcorrelation results will provide insight into the acceleration mechanism of the wind.
Publications	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 The Wide-angle Outflow of the Lensed z = 1.51 AGN HS 0810+2554 \|Chartas G. Cappi M. et al. \| ApJ \| 824-53 \| 2016 \| 2016ApJ...824...53C \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...824...53C 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 The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou Min-Hua Gu Min-Feng \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 Multiphase Powerful Outflows Detected in High-z Quasars \|Chartas G. Cappi M. et al. \| ApJ \| 920-24 \| 2021 \| 2021ApJ...920...24C \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...920...24C Xu2011HESS: A large sample of highly accreting serendipitous AGN under the XMMu2011Newton microscope \|Laurenti M. Tombesi F. et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L 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	2014-10-04T15:44:58Z/2014-10-05T07:33:18Z
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	2015-10-29T23:00:00Z
Last Update	2025-01-27
Keywords	"uv spectral properties", "lensed z", "term variability", "hs0810 makes", "kinetic energy", "120 lensing magnification", "ultrafast outflow", "xray wind properties", "XMM", "feedback mechanisms", "acceleration mechanism", "xray outflow", "agn hs 0810"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr George Chartas, 2015, 'The Ultrafast Outflow of the Lensed z=1.51 AGN HS 0810+2554', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-beclutc