A dataset provided by the European Space Agency

Name: Large Scale ICM Properties of PerseusII - Correcting for Anisotropies
Published: 2007-09-06T00:00:00Z

Proposal ID	040541
Title	Large Scale ICM Properties of PerseusII - Correcting for Anisotropies
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405410101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0405410201
DOI	https://doi.org/10.5270/esa-2pi3i6y
Principal Investigator, PI	Dr Renato Dupke
Abstract	Nearby galaxy clusters present a unique opportunity to study the spatialvariation of the physical properties of the ICM and they also provide templatesto test the biases introduced by simplifications used in the analysis of moredistant clusters. Perseus stands out as the optimal choice for such analysis,due to its brightness, proximity, and ubiquitous physical properties. We propose2 short pointings that, together with other archived ones, will allow us tofully map SN Type enrichment, gas bulk velocities, and other physical parametersup to virgul0.3-0.4 of its virial radius. This analysis will address several currentissues, such as the excess SN Ia pollution in the outer cluster regions and thepresence and extent of ICM velocity gradient.
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 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 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 virgul 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 Automatic Classification of Time-variable X-Ray Sources \|Lo, Kitty K., Farrell, Sean, et al. \| ApJ \| 786-20 \| 2014 \| 2014ApJ...786...20L \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...786...20L 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-Zel.dovich 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 New Sample of Obscured AGNs Selected from the XMM-Newton and AKARI Surveys \|Terashima, Yuichi, Hirata, Yoshitaka, et al. \| ApJ \| 814-11 \| 2015 \| 2015ApJ...814...11T \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...814...11T A novel scenario for the possible X-ray line feature at virgul3.5 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 Way.s 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2006-08-03T07:45:51Z/2006-08-04T02:26:07Z
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	2007-09-06T00:00:00Z
Keywords	"spatial variation", "short pointings", "ubiquitous physical properties", "excesssupernovaia pollution", "outer cluster region", "icm velocity gradient", "nearby galaxy cluster", "perseusii correcting", "perseus stands", "scale icm properties", "biases introduced", "physical properties", "virial radius", "optimal choice", "distant clusters", "gas bulk velocities", "mapsupernovatype enrichment", "physical parameters"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Renato Dupke, 2007, 'Large Scale ICM Properties of PerseusII - Correcting for Anisotropies', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2pi3i6y