|Title||The X-ray Absorber of the X-ray Transint BAL NLS1 WPVS 007|
|Author||Dr Dirk Grupe|
|Description||We propose to obtain a well-exposed X-ray spectrum of the X-ray transient Narrow-Line Seyfert 1 galaxy (NLS1)-transient Broad Absorption-line AGN WPVS 007 with XMM-Newton simultaneously with our approved HST-Chandra observations. The goal is to establish a tight connection between the UV broad absorption line troughs found in FUSE observations and the strong partial covering absorber feature found by Swift. WPVS~007 showed a dramatic transformation into a BAL-QSO between a 1996 HST observation and a 2003 FUSE observation; the recent Swift X-ray detections suggest that the absorber has started to disappear. Therefore it is crucial for our HST COS UV spectroscopy to know what the status of the X-ray absorber is.|
|Publication||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 ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 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 all. . A&A . 595-42 . 2016 . 2016A&A...595A..42T ,
Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity . Ettori, S., Ghirardini, V., et all. . MNRAS . 470-29 . 2017 . 2017MNRAS.470L..29E ,
Reconstruction of the two-dimensional gravitational potential of galaxy clusters from X-ray and Sunyaev-Zel.dovich measurements . Tchernin, C., Bartelmann, M., et all. . A&A . 614-38 . 2018 . 2018A&A...614A..38T ,
The Physics of Galaxy Cluster Outskirts . Walker, Stephen, Simionescu, Aurora, et all. . SSRv . 215-7 . 2019 . 2019SSRv..215....7W ,
|Instrument||EMOS1, EMOS2, EPN, OM, RGS1, RGS2|
|Mission Description||The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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.
|Publisher And Registrant||European Space Agency|
|Credit Guidelines||European Space Agency, 2011-07-03T00:00:00Z, 065190, 17.56_20190403_1200. https://doi.org/10.5270/esa-ty2xdu8|