A dataset provided by the European Space Agency

Name: MAPPING OBSERVATION OF DYNAMICAL STRUCTURES IN THE PERSEUS CLUSTER
Published: 2005-07-04T00:00:00Z

Proposal ID	020472
Title	MAPPING OBSERVATION OF DYNAMICAL STRUCTURES IN THE PERSEUS CLUSTER
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0204720101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0204720201
DOI	https://doi.org/10.5270/esa-5kidqp7
Principal Investigator, PI	Dr TAE FURUSHO
Abstract	X-ray mapping of the Perseus cluster, the brightest cluster in the X-ray sky,with XMM-Newton is the most effective way to study physics of cluster dynamics.In the east region of this cluster, ASCA showed remarkable temperature featuresincluding an enormous cool region bounded by a hot ridge in the east, which ismost possibly caused by a subcluster merger. We propose 7 pointings (including 2pointings of AO2/Pri-C) for a total of 140 ksec to cover most of the unobservedregions in the Perseus cluster, which will give us a detailed view about the gasheating process and metal distribution.
Publications	Radial profiles of Fe abundance in the intracluster medium of nearby clusters observed with XMM-Newton \|Matsushita K. \| A&A \| 527-134 \| 2011 \| 2011A&A...527A.134M \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.134M The XMM-Newton serendipitous survey. V. The Second XMM-Newton serendipitous source catalogue \|Watson M. G. Schroder A. C. et al. \| A&A \| 493-339 \| 2009 \| 2009A&A...493..339W \| http://ui.adsabs.harvard.edu/#abs/2009A&A...493..339W Statistical evaluation of the flux cross-calibration of the XMM-Newton EPIC cameras \|Mateos S. Saxton R. D. et al. \| A&A \| 496-879 \| 2009 \| 2009A&A...496..879M \| http://ui.adsabs.harvard.edu/#abs/2009A&A...496..879M The XMM Cluster Survey: optical analysis methodology and the first data release \|Mehrtens Nicola Romer A. Kathy et al. \| MNRAS \| 423-1024 \| 2012 \| 2012MNRAS.423.1024M \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.1024M An All-Sky Atlas of Radio/X-ray Associations \|Flesch E. \| PASA \| 27-283 \| 2010 \| 2010PASA...27..283F \| http://ui.adsabs.harvard.edu/#abs/2010PASA...27..283F The XMM Cluster Survey: X-ray analysis methodology \|Lloyd-Davies E. J. Romer A. Kathy et al. \| MNRAS \| 418-14 \| 2011 \| 2011MNRAS.418...14L \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.418...14L Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter J. A. Semba S. \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C Classification of X-Ray Sources in the XMM-Newton Serendipitous Source Catalog \|Lin Dacheng Webb Natalie A. \| ApJ \| 756-27 \| 2012 \| 2012ApJ...756...27L \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...756...27L The XMM-Newton serendipitous ultraviolet source survey catalogue \|Page M. J. Brindle C. et al. \| MNRAS \| 426-903 \| 2012 \| 2012MNRAS.426..903P \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.426..903P Ensemble X-ray variability of active galactic nuclei from serendipitous source catalogues \|Vagnetti F. Turriziani S. \| A&A \| 536-84 \| 2011 \| 2011A&A...536A..84V \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..84V Cross-correlation of the 2XMMi catalogue with Data Release 7 of the Sloan Digital Sky Survey \|Pineau F.-X. Motch C. et al. \| A&A \| 527-126 \| 2011 \| 2011A&A...527A.126P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...527A.126P Exploring X-ray and radio emission of type 1 AGN up to z ~ 2.3 \|Ballo L. Heras F. J. H. et al. \| A&A \| 545-66 \| 2012 \| 2012A&A...545A..66B \| http://ui.adsabs.harvard.edu/#abs/2012A&A...545A..66B Large-scale Motions in the Perseus Galaxy Cluster \|Simionescu A. Werner N. et al. \| ApJ \| 757-182 \| 2012 \| 2012ApJ...757..182S \| http://ui.adsabs.harvard.edu/#abs/2012ApJ...757..182S Metal-mass-to-light Ratios of the Perseus Cluster Out to the Virial Radius \|Matsushita K. Sakuma E. et al. \| ApJ \| 764-147 \| 2013 \| 2013ApJ...764..147M \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...764..147M Resonant scattering in the Perseus Cluster: spectral model for constraining gas motions with Astro-H \|Zhuravleva I. Churazov E. et al. \| MNRAS \| 435-3111 \| 2013 \| 2013MNRAS.435.3111Z \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.435.3111Z The diversity of quasars unified by accretion and orientation \|Shen Yue Ho Luis C. \| Natur \| 513-210 \| 2014 \| 2014Natur.513..210S \| http://ui.adsabs.harvard.edu/#abs/2014Natur.513..210S Unidentified Line in X-Ray Spectra of the Andromeda Galaxy and Perseus Galaxy Cluster \|Boyarsky A. Ruchayskiy O. et al. \| PhRvL \| 113-251301 \| 2014 \| 2014PhRvL.113y1301B \| http://ui.adsabs.harvard.edu/#abs/2014PhRvL.113y1301B 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 Sunyaev-Zeldovich effect or not? Detecting the main foreground effect of most galaxy clusters \|Xiao Weike Chen Chen et al. \| MNRAS \| 432-41 \| 2013 \| 2013MNRAS.432L..41X \| http://ui.adsabs.harvard.edu/#abs/2013MNRAS.432L..41X 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 Applications for edge detection techniques using Chandra and XMM-Newton data: galaxy clusters and beyond \|Walker S. A. Sanders J. S. \| MNRAS \| 461-684 \| 2016 \| 2016MNRAS.461..684W \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.461..684W 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 Consistency of Hitomi XMM-Newton and Chandra 3.5 keV data from Perseus \|Conlon Joseph P. Day Francesca et al. \| PhRvD \| 96-123009 \| 2017 \| 2017PhRvD..96l3009C \| http://ui.adsabs.harvard.edu/#abs/2017PhRvD..96l3009C 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 Anisotropy of the galaxy cluster X-ray luminosity-temperature relation \|Migkas Konstantinos Reiprich Thomas H. \| A&A \| 611-50 \| 2018 \| 2018A&A...611A..50M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...611A..50M The split in the ancient cold front in the Perseus cluster \|Walker Stephen A. ZuHone John et al. \| NatAs \| 2-292 \| 2018 \| 2018NatAs...2..292W \| http://ui.adsabs.harvard.edu/#abs/2018NatAs...2..292W 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 Creation of the X-ray sky maps and their application for a search of the dark matter decay line \|Yakubovskyi D. A. Savchenko D. O. \| KosNT \| 21-90 \| 2015 \| 2015KosNT..21e..90Y \| http://ui.adsabs.harvard.edu/#abs/2015KosNT..21e..90Y The XMM Cluster Survey: Present status and latest results \|Viana P. T. P. Mehrtens N. et al. \| AN \| 334-462 \| 2013 \| 2013AN....334..462V \| http://ui.adsabs.harvard.edu/#abs/2013AN....334..462V Testing emergent gravity on galaxy cluster scales \|Tamosiunas Andrius Bacon David et al. \| JCAP \| 5-53 \| 2019 \| 2019JCAP...05..053T \| http://ui.adsabs.harvard.edu/#abs/2019JCAP...05..053T Chandra Follow-up of the SDSS DR8 Redmapper Catalog Using the MATCha Pipeline \|Hollowood Devon L. Jeltema Tesla et al. \| ApJS \| 244-22 \| 2019 \| 2019ApJS..244...22H \| http://ui.adsabs.harvard.edu/#abs/2019ApJS..244...22H Measuring bulk flows of the intracluster medium in the Perseus and Coma galaxy clusters using XMM-Newton \|Sanders J. S. Dennerl K. et al. \| A&A \| 633-42 \| 2020 \| 2020A&A...633A..42S \| http://ui.adsabs.harvard.edu/#abs/2020A&A...633A..42S Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters \|Palmese A. Annis J. et al. \| MNRAS \| 493-4591 \| 2020 \| 2020MNRAS.493.4591P \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.493.4591P The galaxy population within the virial radius of the Perseus cluster \|Meusinger H. Rudolf C. et al. \| A&A \| 640-30 \| 2020 \| 2020A&A...640A..30M \| http://ui.adsabs.harvard.edu/#abs/2020A&A...640A..30M 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 Is There an Enormous Cold Front at the Virial Radius of the Perseus Cluster? \|Walker S. A. Mirakhor M. S. et al. \| ApJ \| 929-37 \| 2022 \| 2022ApJ...929...37W \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...929...37W Baryon cycles in the biggest galaxies \|Donahue Megan Voit G. Mark \| PhR \| 973-1 \| 2022 \| 2022PhR...973....1D \| http://ui.adsabs.harvard.edu/#abs/2022PhR...973....1D 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 A Deep Redshift Survey of the Perseus Cluster (A426): Spatial Distribution and Kinematics of Galaxies \|Kang Wooseok Hwang Ho Seong et al. \| ApJS \| 272-22 \| 2024 \| 2024ApJS..272...22K \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..272...22K 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 X-ray and multiwavelength studies of active galactic nuclei from large area s ky surveys \|Wu Jianfeng \| PhDT \| 0-288 \| 2012 \| 2012PhDT.......288W \| http://ui.adsabs.harvard.edu/#abs/2012PhDT.......288W Hunting dark matter with X-rays \|Franse Jeroen \| PhDT \| 0-148 \| 2016 \| 2016PhDT.......148F \| http://ui.adsabs.harvard.edu/#abs/2016PhDT.......148F Probing the inner Galactic halo with blue horizontal-branch stars. Gaia DR3-based catalogue with atmospheric and stellar parameters \|Culpan R. Dorsch M. et al. \| A&A \| 685-A134 \| 2024 \| 2024A&A...685A.134C \| http://ui.adsabs.harvard.edu/#abs/2024A&A...685A.134C Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M 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	2004-02-04T01:45:49Z/2004-02-04T14:17:48Z
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	2005-07-04T00:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "XMM-Newton", "xray sky", "east region", "hot ridge", "dynamical structures", "xray mapping", "cool region bounded", "xmm newton", "gas heating process", "cluster dynamics", "subcluster merger", "perseus cluster", "brightest cluster", "metal distribution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr TAE FURUSHO, 2005, 'MAPPING OBSERVATION OF DYNAMICAL STRUCTURES IN THE PERSEUS CLUSTER', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-5kidqp7