A dataset provided by the European Space Agency

Name: Witnessing hierarchical structure formation with double &amp; triple galaxy clusters
Published: 2017-01-20T23:00:00Z

Proposal ID	076295
Title	Witnessing hierarchical structure formation with double & triple galaxy clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762950101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762950201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762950301
DOI	https://doi.org/10.5270/esa-47z5ipj
Principal Investigator, PI	Dr Andrea Morandi
Abstract	Double or triple galaxy clusters are unique candidates to observe the processesrelated to individual components at an early stage of merging, such as mutualinteraction between the components, accretion history of the member clusters andthe intercluster medium. We used the metacatalog of X-ray detected clusters ofgalaxies and the Planck cluster catalogue to select a sample of three double andtriple clusters, for which we request XMM time. Through the synergy between XMMand Sunyaev-Zeldovich from Planck, we will recover the thermodynamic propertiesof the gas and constrain accretion processes in the intercluster region. XMMwill therefore play an important role in casting light into these systems andinto the physics at the edge between clusters and large-scale structure filaments.
Publications	Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters \|Lagana, T. F., Durret, F., \| MNRAS \| 484-2807 \| 2019 \| 2019MNRAS.484.2807L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484.2807L The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava, S., Giles, P. A., et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B 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 The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview \|Botteon, A., Shimwell, T. W., et al. \| A&A \| 660-78 \| 2022 \| 2022A&A...660A..78B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium \|Zhang, X., Simionescu, A., et al. \| A&A \| 672-42 \| 2023 \| 2023A&A...672A..42Z \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models \|Cassano, R., Cuciti, V., et al. \| A&A \| 672-43 \| 2023 \| 2023A&A...672A..43C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C Exploring X-Ray Properties of Low-metallicity Dwarf Galaxies \|Cann, Jenna M., Weaver, Kimberly A., et al. \| ApJ \| 961-178 \| 2024 \| 2024ApJ...961..178C \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...961..178C 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2015-05-10T03:52:59Z/2016-01-01T16:14:52Z
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	2017-01-20T23:00:00Z
Keywords	"constrain accretion processes", "triple galaxy cluster", "XMM", "processes related", "intercluster region", "accretion history", "scale structure filaments", "sunyaev zeldovich", "triple clusters", "triple galaxy clusters", "thermodynamic properties", "planck cluster catalogue", "structure formation", "casting light", "intercluster medium", "individual components", "xmm time", "mutual interaction"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Andrea Morandi, 2017, 'Witnessing hierarchical structure formation with double & triple galaxy clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-47z5ipj