A dataset provided by the European Space Agency

Name: Metallicity Profile of A2244, the Brightest Cluster Unobserved with XMM-Newton
Published: 2015-08-25T22:00:00Z

Proposal ID	074090
Title	Metallicity Profile of A2244, the Brightest Cluster Unobserved with XMM-Newton
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0740900101
DOI	https://doi.org/10.5270/esa-12r8jqd
Principal Investigator, PI	Prof Thomas Reiprich
Abstract	The metal abundance profiles in the outskirts of individual galaxy clusters arecurrently mostly unconstrained by observations. These profiles will depend onthe primary enrichment process through cluster galaxies, e.g., ram pressurestripping or galactic super winds. So, measurements can, in principle, constrainwhat the dominant process is. This is the goal of this proposal. We propose ashort supporting XMM-Newton observation of A2244, the brightest cluster in thesky that has not been observed with XMM-Newton until now, to constrain the metalabundance profile out to 0.6 R_180 with a sensational total absolute uncertaintyof Delta Z(0.6 R_180)~0.06 solar using our 70 ks Suzaku observation.
Publications	XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N 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 HICOSMO - cosmology with a complete sample of galaxy clusters - I. Data analysis sample selection and luminosity-mass scaling relation \|Schellenberger G. Reiprich T. H. \| MNRAS \| 469-3738 \| 2017 \| 2017MNRAS.469.3738S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.3738S 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 Connecting optical and X-ray tracers of galaxy cluster relaxation \|Roberts Ian D. Parker Laura C. \| MNRAS \| 475-4704 \| 2018 \| 2018MNRAS.475.4704R \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.4704R 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 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 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 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 On the Reliability of Photometric and Spectroscopic Tracers of Halo Relaxation \|Zhoolideh Haghighi Mohammad H. Raouf Mojtaba et al. \| ApJ \| 904-36 \| 2020 \| 2020ApJ...904...36Z \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...36Z 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 The Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview \|CHEX-MATE Collaboration Arnaud M. et al. \| A&A \| 650-104 \| 2021 \| 2021A&A...650A.104C \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.104C 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 CHEX-MATE: Morphological analysis of the sample \|Campitiello M. G. Ettori S. et al. \| A&A \| 665-117 \| 2022 \| 2022A&A...665A.117C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A.117C 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 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 CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles \|Bartalucci I. Molendi S. et al. \| A&A \| 674-179 \| 2023 \| 2023A&A...674A.179B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A.179B Studying X-ray instruments with galaxy clusters \|Nevalainen J. Molendi S. \| A&A \| 676-142 \| 2023 \| 2023A&A...676A.142N \| http://ui.adsabs.harvard.edu/#abs/2023A&A...676A.142N CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters \|Bourdin H. De Luca F. et al. \| A&A \| 678-181 \| 2023 \| 2023A&A...678A.181B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.181B CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles \|Iqbal A. Pratt G. W. et al. \| A&A \| 679-51 \| 2023 \| 2023A&A...679A..51I \| http://ui.adsabs.harvard.edu/#abs/2023A&A...679A..51I Pressure profiles of distant Galaxy clusters with Planck-SPT data \|Oppizzi Filippo De Luca Federico et al. \| EPJWC \| 257-00035 \| 2022 \| 2022EPJWC.25700035O \| http://ui.adsabs.harvard.edu/#abs/2022EPJWC.25700035O CHEX-MATE: Characterization of the intra-cluster medium temperature distribution \|Lovisari L. Ettori S. et al. \| A&A \| 682-A45 \| 2024 \| 2024A&A...682A..45L \| http://ui.adsabs.harvard.edu/#abs/2024A&A...682A..45L 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 CHEX-MATE: A LOFAR pilot X-ray - radio study on five radio halo clusters \|Balboni M. Gastaldello F. et al. \| A&A \| 686-A5 \| 2024 \| 2024A&A...686A...5B \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A...5B CHEX-MATE: Robust reconstruction of temperature profiles in galaxy clusters with XMM-Newton \|Rossetti M. Eckert D. et al. \| A&A \| 686-A68 \| 2024 \| 2024A&A...686A..68R \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A..68R 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	2014-07-24T04:02:41Z/2014-07-24T11:49:21Z
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	2015-08-25T22:00:00Z
Last Update	2025-01-27
Keywords	"metallicity profile", "delta z0", "06 solar", "xmm newton", "dominant process", "metal abundance profile", "XMM-Newton", "metal abundance profiles", " ram pressure", ".", "cluster galaxy", "XMM", "brightest cluster", "individual galaxy cluster", "primary enrichment process", "galactic super winds"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Thomas Reiprich, 2015, 'Metallicity Profile of A2244, the Brightest Cluster Unobserved with XMM-Newton', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-12r8jqd