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
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	2025-01-27
Keywords	"approved hst", "bal qso", "swift xray detections", "xmm newton", "galaxy nls1", "exposed xray spectrum", "XMM-Newton", "XMM", "tight connection", "1996 hst", "xray absorber", "2003 fuse", "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