A dataset provided by the European Space Agency

Name: XMM survey of the Fornax cluster up to 0.3 of the virial radius
Published: 2010-03-31T00:00:00Z

Proposal ID	055093
Title	XMM survey of the Fornax cluster up to 0.3 of the virial radius
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550930101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550930201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550930301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550930401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550930501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550930601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550930701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550931001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550931201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550931401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0550931601 ...
DOI	https://doi.org/10.5270/esa-ubstkbv
Principal Investigator, PI	Dr Kyoko Matsushita
Abstract	Groups of galaxies and poor clusters of galaxies are best laboratories forstudying history of the universe. The Fornax cluster is the nearest (about 20Mpc) poor cluster with the smallest-iron mass-to-light ratio. In order to studytemperature, entropy and metal distribution and constrain metal enrichment andthermal history in the intracluster medium, we propose to survey the Fornaxcluster up to 0.3 times of the virial radius.
Publications	Suzaku and XMM-Newton Observations of the Fornax Cluster: Temperature and Metallicity Distribution \|Murakami, Hideyoshi, Komiyama, Madoka, et al. \| PASJ \| 63-963 \| 2011 \| 2011PASJ...63S.963M \| http://ui.adsabs.harvard.edu/#abs/2011PASJ...63S.963M 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 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 The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C 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 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 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 SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S Gas Sloshing Regulates and Records the Evolution of the Fornax Cluster \|Su, Yuanyuan, Nulsen, Paul E. J., et al. \| ApJ \| 851-69 \| 2017 \| 2017ApJ...851...69S \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...851...69S The Recent Growth History of the Fornax Cluster Derived from Simultaneous Sloshing and Gas Stripping: Simulating the Infall of NGC 1404 \|Sheardown, Alex, Roediger, Elke, et al. \| ApJ \| 865-118 \| 2018 \| 2018ApJ...865..118S \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...865..118S A new, clean catalogue of extragalactic non-nuclear X-ray sources in nearby galaxies \|Earnshaw, H. P., Roberts, T. P., et al. \| MNRAS \| 483-5554 \| 2019 \| 2019MNRAS.483.5554E \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483.5554E X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C 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 impact of precession on the observed population of ULXs \|Khan, Norman, Middleton, Matthew J., et al. \| MNRAS \| 509-2493 \| 2022 \| 2022MNRAS.509.2493K \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.509.2493K The Redshift Evolution of Ultraluminous X-Ray Sources out to z 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background \|Scott Barrows, R., Comerford, Julia M., et al. \| ApJ \| 932-27 \| 2022 \| 2022ApJ...932...27S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...932...27S CO(J = 1-0) Mapping Survey of 64 Galaxies in the Fornax Cluster with the ALMA Morita Array \|Morokuma-Matsui, Kana, Bekki, Kenji, et al. \| ApJS \| 263-40 \| 2022 \| 2022ApJS..263...40M \| http://ui.adsabs.harvard.edu/#abs/2022ApJS..263...40M 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	2008-06-25T12:32:03Z/2009-02-24T20:20:21Z
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	2010-03-31T00:00:00Z
Keywords	"intracluster medium", "fornax cluster", "XMM", "metal distribution", "xmm survey", "virial radius", "constrain metal enrichment", "iron mass", "thermal history", "light ratio"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Kyoko Matsushita, 2010, 'XMM survey of the Fornax cluster up to 0.3 of the virial radius', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ubstkbv