A dataset provided by the European Space Agency

Name: The X-ray Absorber of the X-ray Transint BAL NLS1 WPVS 007
Published: 2011-07-03T00:00:00Z

Proposal ID	065190
Title	The X-ray Absorber of the X-ray Transint BAL NLS1 WPVS 007
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0651900201
DOI	https://doi.org/10.5270/esa-ty2xdu8
Principal Investigator, PI	Dr Dirk Grupe
Abstract	We propose to obtain a well-exposed X-ray spectrum of the X-ray transientNarrow-Line Seyfert 1 galaxy (NLS1)/transient Broad Absorption-line AGN WPVS 007with XMM-Newton simultaneously with our approved HST/Chandra observations. Thegoal is to establish a tight connection between the UV broad absorption linetroughs found in FUSE observations and the strong partial covering absorberfeature found by Swift. WPVS~007 showed a dramatic transformation into a BAL-QSObetween a 1996 HST observation and a 2003 FUSE observation; the recent SwiftX-ray detections suggest that the absorber has started to disappear. Thereforeit is crucial for our HST COS UV spectroscopy to know what the status of theX-ray absorber is.
Publications	Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov V. N. \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 XMM Cluster Outskirts Project (X-COP): Physical conditions of Abell 2142 up to the virial radius \|Tchernin C. Eckert D. et al. \| A&A \| 595-42 \| 2016 \| 2016A&A...595A..42T \| http://ui.adsabs.harvard.edu/#abs/2016A&A...595A..42T Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity \|Ettori S. Ghirardini V. et al. \| MNRAS \| 470-29 \| 2017 \| 2017MNRAS.470L..29E \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470L..29E Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zeldovich measurements \|Tchernin C. Bartelmann M. et al. \| A&A \| 614-38 \| 2018 \| 2018A&A...614A..38T \| http://ui.adsabs.harvard.edu/#abs/2018A&A...614A..38T The Physics of Galaxy Cluster Outskirts \|Walker Stephen Simionescu Aurora et al. \| SSRv \| 215-7 \| 2019 \| 2019SSRv..215....7W \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215....7W 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 Yet another test of Radial Acceleration Relation for galaxy clusters \|Pradyumna S. Gupta Sajal et al. \| PDU \| 31-100765 \| 2021 \| 2021PDU....3100765P \| http://ui.adsabs.harvard.edu/#abs/2021PDU....3100765P Graviton mass from X-COP galaxy clusters \|Piu00f3rkowska-Kurpas Aleksandra Cao Shuo \| JHEAp \| 33-37 \| 2022 \| 2022JHEAp..33...37P \| http://ui.adsabs.harvard.edu/#abs/2022JHEAp..33...37P Moffats modified gravity tested on X-COP galaxy clusters \|Harikumar Sreekanth Biesiada Marek \| EPJC \| 82-241 \| 2022 \| 2022EPJC...82..241H \| http://ui.adsabs.harvard.edu/#abs/2022EPJC...82..241H The gravitational field of X-COP galaxy clusters \|Eckert D. Ettori S. et al. \| A&A \| 662-123 \| 2022 \| 2022A&A...662A.123E \| http://ui.adsabs.harvard.edu/#abs/2022A&A...662A.123E A test of galaxy cluster fundamental plane for the X-COP sample \|Pradyumna S. Desai Shantanu \| JCAP \| 1-58 \| 2022 \| 2022JCAP...01..058P \| http://ui.adsabs.harvard.edu/#abs/2022JCAP...01..058P A disturbing FABLE of mergers feedback turbulence and mass biases in simulated galaxy clusters \|Bennett Jake S. Sijacki Debora \| MNRAS \| 514-313 \| 2022 \| 2022MNRAS.514..313B \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.514..313B Constraints on dark matter self-interaction from the internal density profiles of X-COP galaxy clusters \|Eckert D. Ettori S. et al. \| A&A \| 666-41 \| 2022 \| 2022A&A...666A..41E \| http://ui.adsabs.harvard.edu/#abs/2022A&A...666A..41E Investigating the turbulent hot gas in X-COP galaxy clusters \|Dupourquu00e9 S. Clerc N. et al. \| A&A \| 673-91 \| 2023 \| 2023A&A...673A..91D \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..91D Testing generalized scalar-tensor theories of gravity with clusters of galaxies \|Haridasu Balakrishna S. Karmakar Purnendu et al. \| PhRvD \| 107-124059 \| 2023 \| 2023PhRvD.107l4059H \| http://ui.adsabs.harvard.edu/#abs/2023PhRvD.107l4059H 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 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	2010-06-11T05:33:11Z/2010-06-12T17:12:17Z
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	2011-07-03T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "swift xray detections", "XMM-Newton", "2003 fuse", "galaxy nls1", "xray absorber", "xmm newton", "tight connection", "bal qso", "approved hst", "1996 hst", "exposed xray spectrum", "HST"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Dirk Grupe, 2011, 'The X-ray Absorber of the X-ray Transint BAL NLS1 WPVS 007', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ty2xdu8