A dataset provided by the European Space Agency

Name: Magnified Views of Relativistic Outflows in Gravitationally Lensed mini-BALQSOs
Published: 2017-02-02T23:00:00Z

Proposal ID	076252
Title	Magnified Views of Relativistic Outflows in Gravitationally Lensed mini-BALQSOs
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762520101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762520201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762520301
DOI	https://doi.org/10.5270/esa-mpm36y3
Principal Investigator, PI	Prof GEORGE CHARTAS
Abstract	We propose to observe three gravitationally lensed mini-BAL quasars. The mainscientific goals are to: (a) Investigate whether relativistic outflows are acommon property of mini-BAL quasars, (b) constrain the properties of theoutflows. These constraints will improve our understanding of the significanceof such outflows in regulating black hole growth and in influencing structureformation, and (c) obtain correlations between the outflow properties of theX-ray absorbers and the X-ray and UV spectral properties of the driving force.These correlations will provide insight into the driving mechanism of quasaroutflows and indicate whether an X-ray absorber is required to drive X-rayand/or UV outflows.
Publications	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 The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava, S., Giles, P. A., et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B 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 X\\u2011HESS: A large sample of highly accreting serendipitous AGN under the XMM\\u2011Newton 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	2015-07-19T20:50:54Z/2016-01-14T05:17:37Z
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	2017-02-02T23:00:00Z
Keywords	"drive xray", "driving mechanism", "xray absorber", "uv spectral properties", "xray absorbers", "regulating blackhole growth", "uv outflows", "mini bal quasars", "magnified views", "main scientific", "quasar outflows", "outflow properties", "driving force", "influencing structure formation", "relativistic outflows"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof GEORGE CHARTAS, 2017, 'Magnified Views of Relativistic Outflows in Gravitationally Lensed mini-BALQSOs', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mpm36y3