A dataset provided by the European Space Agency

Name: Probing the variable, relativistic wind in the high-z QSO HS 1700+6416
Published: 2014-09-05T00:00:00Z

Proposal ID	072370
Title	Probing the variable, relativistic wind in the high-z QSO HS 1700+6416
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723700101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723700201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0723700301
DOI	https://doi.org/10.5270/esa-6aegb7f
Principal Investigator, PI	Dr Giorgio Lanzuisi
Abstract	We propose to perform a monitoring campaign of HS 1700+6416, a luminous NAL-QSOat z=2.735. This remarkable source shows evidences for a broad, high velocity,variable absorption feature in the existing Chandra and XMM spectra. This is thefirst non lensed, high-z QSO with a detected relativistic outflow. The lowquality spectra available, allowed for an estimate of the physical parameters ofthe ionized gas (Lanzuisi et al. 2012). The requested monitoring campaign (340ks observations) will allow to constrain, in each observation, the parametersof the gas within a??5-20%, so that we will be able to study the variability ofthese parameters between observations. This will allow to compute the massoutflow rate/kinetic energy released by the outflow.
Publications	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 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 The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview \|Botteon A. Shimwell T. W. et al. \| A&A \| 660-78 \| 2022 \| 2022A&A...660A..78B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium \|Zhang X. Simionescu A. et al. \| A&A \| 672-42 \| 2023 \| 2023A&A...672A..42Z \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models \|Cassano R. Cuciti V. et al. \| A&A \| 672-43 \| 2023 \| 2023A&A...672A..43C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C 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	2013-05-19T02:24:13Z/2013-08-05T08:57:05Z
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	2014-09-05T00:00:00Z
Last Update	2025-01-27
Keywords	"low quality spectra", "XMM", "xmm spectra", "variable absorption", "luminous nal qso", "z qso", "hs 1700", "ionized gas lanzuisi", "existing chandra", "relativistic wind", "relativistic outflow", "mass outflow rate", "kinetic energy released", "physical parameters"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Giorgio Lanzuisi, 2014, 'Probing the variable, relativistic wind in the high-z QSO HS 1700+6416', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-6aegb7f