We propose to observe 13 nearby edge-on disk galaxies for a total exposure of604ks. These, together with archival data, will enable us to conduct asystematic X-ray survey of 32 such galaxies, which will also be observed withEVLA in an approved 405hr large program. The combination of these radio/X-raydata will enable an unprecedented study of galactic feedback from AGN, SF andevolved stars, particularly in terms of the interplay of hot gas outflows withmagnetic fields and cosmic-rays in regulating the galactic ecosystem.Specifically, we will examine the origins, context and dynamics of the flows andtheir relationships to the galaxy mass, SFR and environment. Understandings ofthese issues in nearby galaxies will serve as a benchmark for the study of similar processes in more distant galaxies.
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function |Vagnetti, F., Middei, R., et al. | A&A | 593-55 | 2016 | 2016A&A...593A..55V | http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V
A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 |Pons, E., Watson, M. G., | A&A | 594-72 | 2016 | 2016A&A...594A..72P | http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P
CHANG-ES - XI. Circular polarization in the cores of nearby galaxies |Irwin, Judith A., Henriksen, Richard N., et al. | MNRAS | 476-5057 | 2018 | 2018MNRAS.476.5057I | http://ui.adsabs.harvard.edu/#abs/2018MNRAS.476.5057I
A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies |Earnshaw, H. P., Roberts, T. P., et al. | MNRAS | 483-5554 | 2019 | 2019MNRAS.483.5554E | http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E
CHANG-ES. XX. High-resolution Radio Continuum Images of Edge-on Galaxies and Their AGNs: Data Release 3 |Irwin, Judith, Wiegert, Theresa, et al. | AJ | 158-21 | 2019 | 2019AJ....158...21I | http://ui.adsabs.harvard.edu/#abs/2019AJ....158...21I
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies |Ojha, Vineet, Chand, Hum, et al. | ApJ | 896-95 | 2020 | 2020ApJ...896...95O | http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O
A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event |Brightman, Murray, Ward, Charlotte, et al. | ApJ | 909-102 | 2021 | 2021ApJ...909..102B | http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B
The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background |Scott Barrows, R., Comerford, Julia M., et al. | ApJ | 932-27 | 2022 | 2022ApJ...932...27S | http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S
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
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
2011-05-05T10:16:00Z/2011-07-18T15:49:40Z
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 Jiang-Tao Li, 2012, 'X-ray Emission from Galaxy Halos --- Circulation and Environmental Effects', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-97l93mw
