A dataset provided by the European Space Agency

Name: Completing the XMM Legacy Mosaic of the Perseus cluster
Published: 2013-03-24T00:00:00Z

Proposal ID	067302
Title	Completing the XMM Legacy Mosaic of the Perseus cluster
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673020201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673020301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0673020401
DOI	https://doi.org/10.5270/esa-abchmbe
Principal Investigator, PI	Dr Daniel Wik
Abstract	XMM-Newton has performed 13 pointing observations of the Perseus cluster (Abell426, z=0.0183), showing remarkable features in the large-scale temperature,pressure, and entropy distributions. Unfortunately, incomplete coverage in theouter east and southeast directions -- coincident with an enigmatic hot regionof unknown origin -- prevents a full characterization of ICM substructure atthese radii. We propose to complete the XMM mosaic of the Perseus cluster withthree 30 ksec pointings. These data will allow us to complete the most detailedinvestigation of cluster substructure known to date, constrain the physicalprocesses -- e.g., merger activity, turbulence, viscosity -- associated with it,and confirm the existence of the eastern hot region detected with ASCA.
Publications	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 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 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 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 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2011-08-19T03:32:51Z/2012-03-01T18:26:14Z
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	2013-03-24T00:00:00Z
Keywords	"perseus cluster", ".", "Abell", "xmm newton", "enigmatic hot region", "hot region", " merger activity", "scale temperature", "entropy distributions", "origin prevents", "physical processes", "XMM", "icm substructure", "XMM-Newton", "outer east", "cluster substructure", "xmm mosaic", "southeast directions coincident", "incomplete coverage"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Daniel Wik, 2013, 'Completing the XMM Legacy Mosaic of the Perseus cluster', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-abchmbe