A dataset provided by the European Space Agency

Name: XMM-Newton Observations of New Massive Planck Clusters
Published: 2017-05-11T22:00:00Z

Proposal ID	076244
Title	XMM-Newton Observations of New Massive Planck Clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762440101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762440201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762440301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762440401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762440501
DOI	https://doi.org/10.5270/esa-cgnozgi
Principal Investigator, PI	Prof John P. Hughes
Abstract	Through a program of ground-based optical and near-infrared imaging begun thisyear, we have identified a number of rich, massive clusters among theunconfirmed Planck cluster candidates. We have selected the five most promisingnew clusters for observation with XMM this cycle. All have Plancksignal-to-noise ratios greater than 5.2 and significant RASS X-ray flux. Theproposed observations will provide the first accurate masses of these clustersbased on multiple X-ray mass proxies and will allow determination of theirdynamical states (merger vs. relaxed systems).
Publications	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 Cluster HEritage project with XMM-Newton: Mass Assembly and Thermodynamics at the Endpoint of structure formation. I. Programme overview \|CHEX-MATE Collaboration Arnaud M. et al. \| A&A \| 650-104 \| 2021 \| 2021A&A...650A.104C \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.104C CHEX-MATE: Morphological analysis of the sample \|Campitiello M. G. Ettori S. et al. \| A&A \| 665-117 \| 2022 \| 2022A&A...665A.117C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A.117C CHEX-MATE: Constraining the origin of the scatter in galaxy cluster radial X-ray surface brightness profiles \|Bartalucci I. Molendi S. et al. \| A&A \| 674-179 \| 2023 \| 2023A&A...674A.179B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A.179B CHEX-MATE: X-ray absorption and molecular content of the interstellar medium toward galaxy clusters \|Bourdin H. De Luca F. et al. \| A&A \| 678-181 \| 2023 \| 2023A&A...678A.181B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...678A.181B Pressure profiles of distant Galaxy clusters with Planck-SPT data \|Oppizzi Filippo De Luca Federico et al. \| EPJWC \| 257-00035 \| 2022 \| 2022EPJWC.25700035O \| http://ui.adsabs.harvard.edu/#abs/2022EPJWC.25700035O 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	2016-01-03T08:34:07Z/2016-04-10T19:32:41Z
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	2017-05-11T22:00:00Z
Last Update	2025-01-27
Keywords	"massive planck clusters", "relaxed systems", "massive cluster", "xmm newton", "rass xray flux", "XMM-Newton", "infrared imaging", "noise ratios", "planck signal", "XMM"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof John P. Hughes, 2017, 'XMM-Newton Observations of New Massive Planck Clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cgnozgi