A dataset provided by the European Space Agency

Name: Filamentary structures within SZ superclusters discovered in the Planck survey
Published: 2013-05-15T00:00:00Z

Proposal ID	067437
Title	Filamentary structures within SZ superclusters discovered in the Planck survey
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674370101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674370201
DOI	https://doi.org/10.5270/esa-hx8v4bg
Principal Investigator, PI	Dr Etienne Pointecouteau
Abstract	We propose a detailed investigation of the nature of two super-structuresdiscovered in the Planck survey and confirmed by XMM-Newton snapshotobservations. We aim at constraining the presence and properties of filamentarystructures connecting and surrounding the clusters. From this jointXMM-Newton/VLT proposal and together with the Planck SZE measurement and alensing analysis, we will unveil the overall dynamics of these two complexstructures and established their detailed pressure distribution. Thus we willperform a direct search for structures in between identified superclusterscomponents from an X-ray/optical analysis, and a careful comparison with precisePlanck SZE measurements.
Publications	Planck intermediate results. VI. The dynamical structure of PLCKG214.6+37.0 a Planck discovered triple system of galaxy clusters \|Planck Collaboration Ade P. A. R. et al. \| A&A \| 550-132 \| 2013 \| 2013A&A...550A.132P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A.132P 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 XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso E. Risaliti G. \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti F. Middei R. et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V 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 Recent Developments in Astrophysical and Cosmological Exploitation of Microwave Surveys \|Burigana Carlo Davies Rodney D. et al. \| IJMPD \| 22-1330011 \| 2013 \| 2013IJMPD..2230011B \| http://ui.adsabs.harvard.edu/#abs/2013IJMPD..2230011B 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 The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava S. Giles P. A. et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman Murray Ward Charlotte et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B 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 X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38 \|Kolodzig Alexander Aghanim Nabila et al. \| A&A \| 653-163 \| 2021 \| 2021A&A...653A.163K \| http://ui.adsabs.harvard.edu/#abs/2021A&A...653A.163K ESASky SSOSS: Solar System Object Search Service and the case of Psyche \|Racero E. Giordano F. et al. \| A&A \| 659-38 \| 2022 \| 2022A&A...659A..38R \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..38R X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf J. Nandra K. et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W A VLT/VIMOS view of two Planck multiple-cluster systems: Structure and galaxy properties \|Wicker R. Aghanim N. et al. \| A&A \| 676-61 \| 2023 \| 2023A&A...676A..61W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...676A..61W 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	2011-05-25T00:48:02Z/2012-04-26T12:47:38Z
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	2013-05-15T00:00:00Z
Last Update	2025-01-27
Keywords	"super structures", "overall dynamics", "complex structures", "sz superclusters", "xmm newton", "planck survey", "optical analysis", "XMM-Newton", "filamentary structures connecting", "lensing analysis", "pressure distribution", "XMM", "superclusters components", "xmm newton snapshot", "filamentary structures", "planck sze measurement"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Etienne Pointecouteau, 2013, 'Filamentary structures within SZ superclusters discovered in the Planck survey', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hx8v4bg