A dataset provided by the European Space Agency

Name: Probing the interplay between the intragroup medium and galaxies with XMM
Published: 2012-05-10T00:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

Proposal ID	065530
Title	Probing the interplay between the intragroup medium and galaxies with XMM
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655300101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655300301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655300601
DOI	https://doi.org/10.5270/esa-j2u0uqh
Principal Investigator, PI	Dr Francesco Miniati
Abstract	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 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 \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y 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 The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Classification of 4XMM-DR9 sources by machine learning \|Zhang Yanxia Zhao Yongheng \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan Z. S. Han J. L. \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y The alignment between brightest cluster galaxies and host clusters \|Yuan Z. S. Wen Z. L. \| MNRAS \| 516-3159 \| 2022 \| 2022MNRAS.516.3159Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.516.3159Y Dynamical Response of Solar Wind Charge Exchange Soft X-Ray Emission in Earths 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 \|Lourenu00e7o Ana C. C. Jaffu00e9 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 From Active Stars to Black Holes: A Discovery Tool for Galactic X-Ray Sources \|Rodriguez Antonio C. \| PASP \| 136-054201 \| 2024 \| 2024PASP..136e4201R \| http://ui.adsabs.harvard.edu/#abs/2024PASP..136e4201R 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2010-05-22T22:33:42Z/2011-04-23T07:08:03Z
Version	21.51_20241115_1113
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.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2012-05-10T00:00:00Z
Last Update	2026-07-09
Keywords	"agn populations", "agn andsupernovafeedback", "XMM-Newton", "physical processes", "ordinary intermediate density", "intragroup medium", "XMM", "galaxy feedback", "xmm xray data", "ram pressure", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Francesco Miniati, 2012, 'Probing the interplay between the intragroup medium and galaxies with XMM', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-j2u0uqh
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.