The success of current galaxy evolution models hinges critically on the role ofAGN and SN feedback. We propose for X-ray observations with XMM-Newton to study20 galaxy groups in ZENS with known galaxy and AGN populations to test the roleof AGN and galaxy feedback in such models. The proposed XMM X-ray data will alsoquantify to what extent the intra-group medium affects galaxy evolution, in theordinary intermediate-density environment of galaxy groups, through physicalprocesses such as ram pressure and strangulation.
Publications
The X-Ray Zurich Environmental Study (X-ZENS). I. Chandra and XMM-Newton Observations of Active Galactic Nuclei in Galaxies in nearby Groups |Silverman, J. D., Miniati, F., et al. | ApJ | 780-67 | 2014 | 2014ApJ...780...67S | http://ui.adsabs.harvard.edu/#abs/2014ApJ...780...67S
The X-Ray Zurich Environmental Study (X-ZENS). II. X-Ray Observations of the Diffuse Intragroup Medium in Galaxy Groups |Miniati, Francesco, Finoguenov, Alexis, et al. | ApJ | 819-26 | 2016 | 2016ApJ...819...26M | http://ui.adsabs.harvard.edu/#abs/2016ApJ...819...26M
Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earth.s Magnetosphere to the Solar Wind Proton Flux |Zhang, Yingjie, Sun, Tianran, et al. | ApJ | 948-69 | 2023 | 2023ApJ...948...69Z | http://ui.adsabs.harvard.edu/#abs/2023ApJ...948...69Z
More relaxed intracluster gas than galaxies in clusters in quasi-equilibrium |Yuan, Z. S., Han, J. L., et al. | MNRAS | 523-1364 | 2023 | 2023MNRAS.523.1364Y | http://ui.adsabs.harvard.edu/#abs/2023MNRAS.523.1364Y
The effect of cluster dynamical state on ram-pressure stripping |Louren\\u00e7o, Ana C. C., Jaff\\u00e9, Y. L., et al. | MNRAS | 526-4831 | 2023 | 2023MNRAS.526.4831L | http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.4831L
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
Distribution of Merging and Post-merger Galaxies in Nearby Galaxy Clusters |Kim, Duho, Sheen, Yun-Kyeong, et al. | ApJ | 966-124 | 2024 | 2024ApJ...966..124K | http://ui.adsabs.harvard.edu/#abs/2024ApJ...966..124K
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
2010-05-22T22:33:42Z/2011-04-23T07:08:03Z
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 Francesco Miniati, 2012, 'Probing the interplay between the intragroup medium and galaxies with XMM', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-j2u0uqh
