|Title||X-ray properties of Zw 229.015, a Seyfert 1 AGN in the Kepler field|
|Author||Prof Luigi Gallo|
|Description||The Seyfert 1 galaxy Zw 229.015 is an anonymous, unstudied AGN near the galactic plane, but by virtue of being in the Kepler field of view it will have the most precise, long-term optical light curve of any AGN ever. As such, the AGN is the ideal candidate for reverberation-echo mapping studies and will be the target of such an investigation in 2011 and 2012. However, there is almost nothing known about the X-ray properties of this AGN: Zw 229 has never been the focus of a targeted observation and has only been detected in the RASS. In AO10 our intention is simply to characterize the X-ray properties and behavior of Zw 229. We propose three observations of Zw 229 over the course of AO10 to measure the object.s X-ray spectrum and determine its long- and short-time scale spectral variability.|
|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 ,
A hard X-ray view of the soft excess in AGN . Boissay, Rozenn, Ricci, Claudio, . A&A . 588-70 . 2016 . 2016A&A...588A..70B ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
Spectral and time series analyses of the Seyfert 1 AGN: Zw 229.015 . Adegoke, Oluwashina, Rakshit, Suvendu, . MNRAS . 466-3951 . 2017 . 2017MNRAS.466.3951A ,
AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton . Svoboda, J., Guainazzi, M., . A&A . 603-127 . 2017 . 2017A&A...603A.127S ,
The nature of the soft excess and spectral variability in the Seyfert 1 galaxy Zw 229.015 . Tripathi, S., Waddell, S. G. H., et all. . MNRAS . 488-4831 . 2019 . 2019MNRAS.488.4831T ,
Activity and rotation of the X-ray emitting Kepler stars . Pizzocaro, D., Stelzer, B., et all. . A&A . 628-41 . 2019 . 2019A&A...628A..41P ,
|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, 2012-06-24T00:00:00Z, 067253, 17.56_20190403_1200. https://doi.org/10.5270/esa-zyeyh0m|