A dataset provided by the European Space Agency

Name: X-Ray Luminosity--Mass Relation and AGN Feedback in Galaxy Groups
Published: 2011-10-27T00:00:00Z

Proposal ID	065358
Title	X-Ray Luminosity--Mass Relation and AGN Feedback in Galaxy Groups
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653580101
DOI	https://doi.org/10.5270/esa-nu96n8s
Principal Investigator, PI	Dr Thomas Reiprich
Abstract	Most of the mass, most of the baryons, and most of the galaxies in the Universeare in galaxy groups. The processes connecting cooling gas in the hot inter-galactic medium and feedback from AGN are more easily observed in groups than inclusters because of their shallower potential wells. A precise characterizationof the X-ray luminosity-mass relation over a large mass range is todays singlemost important task to ensure that the full cosmological power from the 100000groups and clusters to be detected with eROSITA can be exploited. We will use acomplete sample of almost 90 galaxy groups and clusters to constrain cooling andfeedback mechanisms as well as the Lx-M relation. Observations for all clustersare available. With this short proposal we aim to complete observations for the group sample.
Publications	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 Scaling properties of a complete X-ray selected galaxy group sample \|Lovisari L. Reiprich T. H. \| A&A \| 573-118 \| 2015 \| 2015A&A...573A.118L \| http://ui.adsabs.harvard.edu/#abs/2015A&A...573A.118L 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 The non-uniformity of galaxy cluster metallicity profiles \|Lovisari L. Reiprich T. H. \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L Effect of interacting dark energy on mass-temperature relation in galaxy clusters \|Naseri Mahdi Firouzjaee Javad T. \| PhRvD \| 102-123503 \| 2020 \| 2020PhRvD.102l3503N \| http://ui.adsabs.harvard.edu/#abs/2020PhRvD.102l3503N Scaling Properties of Galaxy Groups \|Lovisari Lorenzo Ettori Stefano et al. \| Univ \| 7-139 \| 2021 \| 2021Univ....7..139L \| http://ui.adsabs.harvard.edu/#abs/2021Univ....7..139L 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 Galaxy Groups as the Ultimate Probe of AGN Feedback \|Eckert Dominique Gastaldello Fabio et al. \| Galax \| 12-24 \| 2024 \| 2024Galax..12...24E \| http://ui.adsabs.harvard.edu/#abs/2024Galax..12...24E 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	2010-10-02T00:54:35Z/2010-10-02T11:22:24Z
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.
Creator Contact	https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published	2011-10-27T00:00:00Z
Last Update	2025-01-27
Keywords	"cosmological power", "complete sample", "constrain cooling", "mass range", "shallower potential", "precise characterization", "feedback mechanisms", "agn feedback"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Thomas Reiprich, 2011, 'X-Ray Luminosity--Mass Relation and AGN Feedback in Galaxy Groups', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-nu96n8s