A dataset provided by the European Space Agency

Name: Probing the matter flow in distant QSO with the aid of gravitational lensing
Published: 2018-03-30T22:00:00Z

Proposal ID	078121
Title	Probing the matter flow in distant QSO with the aid of gravitational lensing
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781210201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0781210301
DOI	https://doi.org/10.5270/esa-lha5kd4
Principal Investigator, PI	Dr Mauro Dadina
Abstract	The M_SMBH-sigma relation proved that the central black-hole and the hostinggalaxies co-evolved across cosmic time. The X-ray ultra-fast outflows in nearbyAGN, are probably one of the ingredients that built-up the needed feedbackmechanism. At high-z, however, they were measured only in few objects, mainlythanks to gravitational lenses. We thus propose to continue a program started inXMM-Newton AO13, to point for 150 and 80 ks a couple of distant and lensed QSO:Q2237+030 and MG0414+0534. Our goal is to characterize their X-ray spectrum andto detect blushifted absorption lines at E$sim$7-9 keV and, possibly, blurredreflection component.
Publications	Yet another UFO in the X-ray spectrum of a high-z lensed QSO \|Dadina M. Vignali C. et al. \| A&A \| 610-13 \| 2018 \| 2018A&A...610L..13D \| http://ui.adsabs.harvard.edu/#abs/2018A&A...610L..13D X-raying winds in distant quasars: The first high-redshift wind duty cycle \|Bertola E. Dadina M. et al. \| A&A \| 638-136 \| 2020 \| 2020A&A...638A.136B \| http://ui.adsabs.harvard.edu/#abs/2020A&A...638A.136B 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 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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M 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	2016-11-26T19:27:26Z/2017-03-12T18:43:10Z
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	2018-03-30T22:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "galaxy co evolved", "blushifted absorption lines", "matter flow", "XMM-Newton", "cosmic time", "central blackhole", "distant qso", "gravitational lens", "lensed qso", "blurred reflection component", "feedback mechanism", "xmm newton ao13", "xray spectrum", "nearby agn", "program started"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Mauro Dadina, 2018, 'Probing the matter flow in distant QSO with the aid of gravitational lensing', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-lha5kd4