A dataset provided by the European Space Agency

Name: A detailed study of the most powerful radio halo cluster with XMM-Newton
Published: 2012-11-01T00:00:00Z

Proposal ID	067242
Title	A detailed study of the most powerful radio halo cluster with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672420101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672420201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0672420301
DOI	https://doi.org/10.5270/esa-ghvskup
Principal Investigator, PI	Dr Evan Million
Abstract	We propose an XMM-Newton observation of the galaxy cluster MACS,J0717.5+3745(z=0.546), which contains the most powerful and highest redshift radio haloknown. We will map in detail the complex thermodynamics of this spectaculartriple merger system, and probe the connection between the X-ray emitting,thermal gas and the radio bright, non-thermal particle population.
Publications	A Measurement of the Kinetic Sunyaev-Zeldovich Signal Toward MACS J0717.5+3745 \|Sayers J. Mroczkowski T. et al. \| ApJ \| 778-52 \| 2013 \| 2013ApJ...778...52S \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...778...52S CLASH: Complete Lensing Analysis of the Largest Cosmic Lens MACS J0717.5+3745 and Surrounding Structures \|Medezinski Elinor Umetsu Keiichi et al. \| ApJ \| 777-43 \| 2013 \| 2013ApJ...777...43M \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...777...43M Scaling Relations and X-Ray Properties of Moderate-luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton \|Connor Thomas Donahue Megan et al. \| ApJ \| 794-48 \| 2014 \| 2014ApJ...794...48C \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...794...48C 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 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 Mapping the kinetic Sunyaev-Zeldovich effect toward MACS J0717.5+3745 with NIKA \|Adam R. Bartalucci I. et al. \| A&A \| 598-115 \| 2017 \| 2017A&A...598A.115A \| http://ui.adsabs.harvard.edu/#abs/2017A&A...598A.115A Pressure Profiles of Distant Galaxy Clusters in the Planck Catalogue \|Bourdin H. Mazzotta P. et al. \| ApJ \| 843-72 \| 2017 \| 2017ApJ...843...72B \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...843...72B X-Ray Morphological Analysis of the Planck ESZ Clusters \|Lovisari Lorenzo Forman William R. et al. \| ApJ \| 846-51 \| 2017 \| 2017ApJ...846...51L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...846...51L Mapping the hot gas temperature in galaxy clusters using X-ray and Sunyaev-Zeldovich imaging \|Adam R. Arnaud M. et al. \| A&A \| 606-64 \| 2017 \| 2017A&A...606A..64A \| http://ui.adsabs.harvard.edu/#abs/2017A&A...606A..64A Recovering galaxy cluster gas density profiles with XMM-Newton and Chandra \|Bartalucci I. Arnaud M. et al. \| A&A \| 608-88 \| 2017 \| 2017A&A...608A..88B \| http://ui.adsabs.harvard.edu/#abs/2017A&A...608A..88B The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching \|van der Burg Remco F. J. McGee Sean et al. \| A&A \| 618-140 \| 2018 \| 2018A&A...618A.140V \| http://ui.adsabs.harvard.edu/#abs/2018A&A...618A.140V Growing a cosmic beast: observations and simulations of MACS J0717.5+3745 \|Jauzac M. Eckert D. et al. \| MNRAS \| 481-2901 \| 2018 \| 2018MNRAS.481.2901J \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.481.2901J Astrophysics with the Spatially and Spectrally Resolved Sunyaev-Zeldovich Effects. A Millimetre/Submillimetre Probe of the Warm and Hot Universe \|Mroczkowski Tony Nagai Daisuke et al. \| SSRv \| 215-17 \| 2019 \| 2019SSRv..215...17M \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215...17M The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state \|Bartalucci I. Arnaud M. et al. \| A&A \| 628-86 \| 2019 \| 2019A&A...628A..86B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..86B X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton \|Lovisari Lorenzo Schellenberger Gerrit et al. \| ApJ \| 892-102 \| 2020 \| 2020ApJ...892..102L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L The BUFFALO HST Survey \|Steinhardt Charles L. Jauzac Mathilde et al. \| ApJS \| 247-64 \| 2020 \| 2020ApJS..247...64S \| http://ui.adsabs.harvard.edu/#abs/2020ApJS..247...64S Comparing different mass estimators for a large subsample of the Planck-ESZ clusters \|Lovisari L. Ettori S. et al. \| A&A \| 644-78 \| 2020 \| 2020A&A...644A..78L \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L The thermalization of massive galaxy clusters \|Sereno Mauro Lovisari Lorenzo et al. \| MNRAS \| 507-5214 \| 2021 \| 2021MNRAS.507.5214S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5214S 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 Linking a universal gas density profile to the core-excised X-ray luminosity in galaxy clusters up to z u223c 1.1 \|Pratt G. W. Arnaud M. et al. \| A&A \| 665-24 \| 2022 \| 2022A&A...665A..24P \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A..24P Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters \|Wicker R. Douspis M. et al. \| A&A \| 674-48 \| 2023 \| 2023A&A...674A..48W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W 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	2011-10-11T17:20:20Z/2011-10-16T09:46:25Z
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	2012-11-01T00:00:00Z
Last Update	2025-01-27
Keywords	"J0717.5", "radio bright", "thermal gas", "complex thermodynamics", "3745 z", "xmm newton", "XMM-Newton", "redshift radio halo", "galaxy cluster macs", "xray emitting", "nonthermal particle population", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Evan Million, 2012, 'A detailed study of the most powerful radio halo cluster with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ghvskup