|Title||Tracking down the AGN in galaxies with massive molecular outflows|
|Author||Dr Enrico Piconcelli|
|Description||We propose uninterrupted 120 ks observations of two nearby sources wherein the presence of a massive molecular outflow has been recently discovered. These objects stand out for being peculiar cases in the current theoretical framework of the AGN feedback scenario. Our goal is to constrain the physical properties (luminosity, obscuration) of the likely primary driver of these giant outflows, i.e the central AGN, via deep X-ray spectroscopy of unprecedented quality. Thanks to the large collecting area and large visibility windows, XMM-Newton is the most suitable X-ray mission for carrying out the proposed study.|
|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 ,
Suppression of Star Formation in NGC 1266 . Alatalo, Katherine, Lacy, Mark, et all. . ApJ . 798-31 . 2015 . 2015ApJ...798...31A ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
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 ,
A Study of X-Ray Emission of Galaxies Hosting Molecular Outflows (MOX Sample) . Laha, Sibasish, Guainazzi, Matteo, et all. . ApJ . 868-10 . 2018 . 2018ApJ...868...10L ,
Kinetic Energy Transfer from X-Ray Ultrafast Outflows to Millimeter-Submillimeter Cold Molecular Outflows in Seyfert Galaxies . Mizumoto, Misaki, Izumi, Takuma, . ApJ . 871-156 . 2019 . 2019ApJ...871..156M ,
|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, 2014-03-21T00:00:00Z, 069352, 17.56_20190403_1200. https://doi.org/10.5270/esa-n4ch8y7|