A dataset provided by the European Space Agency

Name: First detailed metallicity map of a merging galaxy cluster: Abell 2319
Published: 2010-12-18T00:00:00Z

Proposal ID	060004
Title	First detailed metallicity map of a merging galaxy cluster: Abell 2319
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0600040101
DOI	https://doi.org/10.5270/esa-5b6wrg3
Principal Investigator, PI	Prof Sabine Schindler
Abstract	We propose to observe the bright nearby merging cluster Abell 2319 whichexhibits an extended and powerful radio halo with an irregular morphology wellcorrelated with a strong asymmetry in its X-ray brightness. With the requestedobservation we aim to: 1) derive the metallicity map in order to study the metaldistributions of a merging cluster up to the outer region; 2) compare thismetallicity map with those obtained from our simulations; 3) study thecorrelations between X-ray, radio and optical properties and investigate thenature of the extended radio emission; 4) measure the relative abundance of ironwith respect to elements in order to constrain the relative fraction of Type IIand Type Ia SNe.
Publications	Detection of an Unidentified Emission Line in the Stacked X-Ray Spectrum of Galaxy Clusters \|Bulbul Esra Markevitch Maxim et al. \| ApJ \| 789-13 \| 2014 \| 2014ApJ...789...13B \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...789...13B 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 A radio and X-ray study of the merging cluster A2319 \|Storm Emma Jeltema Tesla E. \| MNRAS \| 448-2495 \| 2015 \| 2015MNRAS.448.2495S \| http://ui.adsabs.harvard.edu/#abs/2015MNRAS.448.2495S Where do the 3.5 keV photons come from? A morphological study of the Galactic Center and of Perseus \|Carlson Eric Jeltema Tesla \| JCAP \| 2-9 \| 2015 \| 2015JCAP...02..009C \| http://ui.adsabs.harvard.edu/#abs/2015JCAP...02..009C A novel scenario for the possible X-ray line feature at ~3.5 keV. Charge exchange with bare sulfur ions \|Gu L. Kaastra J. et al. \| A&A \| 584-11 \| 2015 \| 2015A&A...584L..11G \| http://ui.adsabs.harvard.edu/#abs/2015A&A...584L..11G 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 Dark matter distribution in X-ray luminous galaxy clusters with Emergent Gravity \|Ettori S. Ghirardini V. et al. \| MNRAS \| 470-29 \| 2017 \| 2017MNRAS.470L..29E \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.470L..29E X-Ray Lines from Dark Matter Annihilation at the keV Scale \|Brdar Vedran Kopp Joachim et al. \| PhRvL \| 120-61301 \| 2018 \| 2018PhRvL.120f1301B \| http://ui.adsabs.harvard.edu/#abs/2018PhRvL.120f1301B WIMP dark matter candidates and searches---current status and future prospects \|Roszkowski Leszek Sessolo Enrico Maria \| RPPh \| 81-66201 \| 2018 \| 2018RPPh...81f6201R \| http://ui.adsabs.harvard.edu/#abs/2018RPPh...81f6201R Resonantly Produced 7A keV Sterile Neutrino Dark Matter Models and the Properties of Milky Way Satellites \|Abazajian Kevork N. \| PhRvL \| 112-161303 \| 2014 \| 2014PhRvL.112p1303A \| http://ui.adsabs.harvard.edu/#abs/2014PhRvL.112p1303A The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the intracluster medium out to R200 in Abell 2319 \|Ghirardini V. Ettori S. et al. \| A&A \| 614-7 \| 2018 \| 2018A&A...614A...7G \| http://ui.adsabs.harvard.edu/#abs/2018A&A...614A...7G 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 Thermodynamic profiles of galaxy clusters from a joint X-ray/SZ analysis \|Shitanishi Jennifer A. Pierpaoli Elena et al. \| MNRAS \| 481-749 \| 2018 \| 2018MNRAS.481..749S \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.481..749S Laboratory Measurements of X-Ray Emission from Highly Charged Argon Ions \|Bulbul Esra Foster Adam et al. \| ApJ \| 870-21 \| 2019 \| 2019ApJ...870...21B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...870...21B Activity and rotation of the X-ray emitting Kepler stars \|Pizzocaro D. Stelzer B. et al. \| A&A \| 628-41 \| 2019 \| 2019A&A...628A..41P \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..41P Iron in X-COP: Tracing enrichment in cluster outskirts with high accuracy abundance profiles \|Ghizzardi Simona Molendi Silvano et al. \| A&A \| 646-92 \| 2021 \| 2021A&A...646A..92G \| http://ui.adsabs.harvard.edu/#abs/2021A&A...646A..92G Metastable conformal dark matter \|Brax Philippe Kaneta Kunio et al. \| PhRvD \| 103-115016 \| 2021 \| 2021PhRvD.103k5016B \| http://ui.adsabs.harvard.edu/#abs/2021PhRvD.103k5016B A Search for the 3.5 keV Line from the Milky Ways Dark Matter Halo with HaloSat \|Silich E. M. Jahoda K. et al. \| ApJ \| 916-2 \| 2021 \| 2021ApJ...916....2S \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...916....2S 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 Stellar Superflares Observed Simultaneously with Kepler and XMM-Newton \|Kuznetsov Alexey A. Kolotkov Dmitrii Y. \| ApJ \| 912-81 \| 2021 \| 2021ApJ...912...81K \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...81K 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 Multiwavelength Quasi-periodic Pulsations in a Stellar Superflare \|Kolotkov Dmitrii Y. Nakariakov Valery M. et al. \| ApJ \| 923-33 \| 2021 \| 2021ApJ...923L..33K \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...923L..33K 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 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 Flares and rotation of M dwarfs with habitable zones accessible to TESS planet detections \|Stelzer B. Bogner M. et al. \| A&A \| 665-30 \| 2022 \| 2022A&A...665A..30S \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A..30S 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 Possible Detection of a Flare-associated Coronal Mass Ejection on an M-dwarf \|Wang J. \| RAA \| 23-95019 \| 2023 \| 2023RAA....23i5019W \| http://ui.adsabs.harvard.edu/#abs/2023RAA....23i5019W 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 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 Was There a 3.5 keV Line? \|Dessert Christopher Foster Joshua W. et al. \| ApJ \| 964-185 \| 2024 \| 2024ApJ...964..185D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...964..185D 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 Nonthermal Emission from Galaxy Clusters \|Storm Emma \| PhDT \| 0-149 \| 2015 \| 2015PhDT.......149S \| http://ui.adsabs.harvard.edu/#abs/2015PhDT.......149S CHEX-MATE: Turbulence in the intra-cluster medium from X-ray surface brightness fluctuations \|Dupourquu00e9 S. Clerc N. et al. \| A&A \| 687-A58 \| 2024 \| 2024A&A...687A..58D \| http://ui.adsabs.harvard.edu/#abs/2024A&A...687A..58D 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	2009-11-29T20:20:06Z/2009-11-30T12:32:03Z
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	2010-12-18T00:00:00Z
Last Update	2025-08-04
Keywords	"abell 2319", "powerful radio halo", "relative fraction", "optical properties", "type ia sne", "merging cluster", "metal distributions", "radio emission", "Abell 2319", "relative abundance", "metallicity map", "xray brightness", "outer region", "irregular morphology", "type ii", "merging galaxy cluster"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Sabine Schindler, 2010, 'First detailed metallicity map of a merging galaxy cluster: Abell 2319', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5b6wrg3