We propose simultaneous 200 ks XMM-Newton-RGS and HST-COS observations of thenarrow line Seyfert1 IZw1. We will study the connection between the X-ray and UVabsorber, mapping the ionization structure, kinematic behavior and elementalabundances. Finally we will quantify the AGN feedback by directly measuring themetal enrichment by C, N, O, and Fe and the kinetic luminosity of the outflow.
Publications
Revealing structure and evolution within the corona of the Seyfert galaxy I Zw 1 |Wilkins, D. R., Gallo, L. C., et al. | MNRAS | 471-4436 | 2017 | 2017MNRAS.471.4436W | http://ui.adsabs.harvard.edu/#abs/2017MNRAS.471.4436W
The variability of the warm absorber in I Zwicky 1 as seen by XMM-Newton |Silva, C. V., Costantini, E., et al. | MNRAS | 480-2334 | 2018 | 2018MNRAS.480.2334S | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.480.2334S
A Study of X-Ray Emission of Galaxies Hosting Molecular Outflows (MOX Sample) |Laha, Sibasish, Guainazzi, Matteo, et al. | ApJ | 868-10 | 2018 | 2018ApJ...868...10L | http://ui.adsabs.harvard.edu/#abs/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 | http://ui.adsabs.harvard.edu/#abs/2019ApJ...871..156M
Constraining energy-dependent emissivity profiles of AGN inflows |Ashton, Dominic I., Middleton, Matthew J., | MNRAS | 513-5245 | 2022 | 2022MNRAS.513.5245A | http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.5245A
A Systematic Study of the Short-term X-Ray Variability of Seyfert Galaxies. I. Diversity of the X-Ray rms Spectra |Hu, Jingwei, Jin, Chichuan, et al. | ApJ | 936-105 | 2022 | 2022ApJ...936..105H | http://ui.adsabs.harvard.edu/#abs/2022ApJ...936..105H
X\\u2011HESS: A large sample of highly accreting serendipitous AGN under the XMM\\u2011Newton microscope |Laurenti, M., Tombesi, F., et al. | AN | 344-20230053 | 2023 | 2023AN....34430053L | http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L
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
Tracing the evolving X-ray reverberation lags within an individual AGN light curve |Nakhonthong, N., Chainakun, P., et al. | MNRAS | 530-1894 | 2024 | 2024MNRAS.530.1894N | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.530.1894N
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
2015-01-19T08:55:52Z/2015-01-22T22:40:13Z
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.
European Space Agency, Dr Elisa Costantini, 2016, 'Feedback in action in the type 1 Seyfert IZw 1', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-v0ywwc4
