A dataset provided by the European Space Agency

Name: X-ray large scale survey of the nearby galaxy cluster Abell2199
Published: 2018-04-19T22:00:00Z

Proposal ID	078452
Title	X-ray large scale survey of the nearby galaxy cluster Abell2199
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784520101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0784521701
DOI	https://doi.org/10.5270/esa-be2o7em
Principal Investigator, PI	Dr Takayuki Tamura
Abstract	We use XMM to map the cluster Abell 2199 intermediate region (<3/4 virialradius) and search X-ray faint substructures in a wide spacial range from agalaxy to a cluster and larger sizes. We observed this area with SUZAKU andfound a number of structures and a hint of asymmetric large scale emission.These substructures along with unresolved background sources should be resolvedspatially and covered fully with XMM imaging. Errors of the EPIC background willbe reduced by our SUZAKU deep spectra. These X-ray maps will be compared withour wide area weak-lensing data observed with SUBARU Hyper suprime-Cam. The XMMobservations provide uniquely a direct comparison among structures of galaxies,ICM, and dark matter.
Publications	A high coverage view of the thermodynamics and metal abundance in the outskirts of the nearby galaxy cluster Abell 2199 \|Mirakhor M. S. Walker S. A. \| MNRAS \| 497-3943 \| 2020 \| 2020MNRAS.497.3943M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3943M 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 X-ray view of optically selected dual AGN \|De Rosa Alessandra Vignali Cristian et al. \| MNRAS \| 519-5149 \| 2023 \| 2023MNRAS.519.5149D \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.519.5149D Dashing through the cluster: An X-ray to radio view of UGC 10420 undergoing ram-pressure stripping \|Mahajan Smriti Singh Kulinder Pal et al. \| PASA \| 40-9 \| 2023 \| 2023PASA...40....9M \| http://ui.adsabs.harvard.edu/#abs/2023PASA...40....9M Xu2011HESS: A large sample of highly accreting serendipitous AGN under the XMMu2011Newton microscope \|Laurenti M. Tombesi F. et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L A Surprising Periodicity Detected during a Super-outburst of V844 Herculis by TESS \|Greiveldinger Anousha Garnavich Peter et al. \| ApJ \| 955-150 \| 2023 \| 2023ApJ...955..150G \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...955..150G The XMM-Newton Line Emission Analysis Program (X-LEAP). I. Emission-line Survey of O VII O VIII and Fe L-shell Transitions \|Pan Zeyang Qu Zhijie et al. \| ApJS \| 271-62 \| 2024 \| 2024ApJS..271...62P \| http://ui.adsabs.harvard.edu/#abs/2024ApJS..271...62P 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2017-03-03T07:00:31Z/2017-03-22T10:50:54Z
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	2018-04-19T22:00:00Z
Last Update	2025-01-27
Keywords	"Abell2199", "virial radius", "xmm imaging", "EPIC", "suzaku deep spectra", "scale emission", "wide spacial range", "xray maps", "scale survey", "larger sizes", "x ray", "weak lensing data", "dark matter", "XMM", "unresolved background sources", "epic background"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Takayuki Tamura, 2018, 'X-ray large scale survey of the nearby galaxy cluster Abell2199', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-be2o7em