A dataset provided by the European Space Agency

Name: Probing the extreme mass peaks at z>0.7
Published: 2018-03-29T22:00:00Z

Proposal ID	078388
Title	Probing the extreme mass peaks at z>0.7
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783880901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783881001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783881201 ... https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783881301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783881401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783881701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0783881901
DOI	https://doi.org/10.5270/esa-86wsowh
Principal Investigator, PI	Dr Monique Arnaud
Abstract	We propose to obtain spatially resolved X-ray spectroscopy of a sample of 20massive (M>5e+14M_sun) clusters detected blindly by Planck in the redshift range0.7
Publications	Searching for gamma-ray signature in WHSP blazars. Fermi-LAT detection of 150 excess signal in the 0.3-500 GeV band \|Arsioli B. Chang Y.-L. \| A&A \| 598-134 \| 2017 \| 2017A&A...598A.134A \| http://ui.adsabs.harvard.edu/#abs/2017A&A...598A.134A A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha Vineet Chand Hum et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O Fast magnetic field amplification in distant galaxy clusters \|Di Gennaro Gabriella van Weeren Reinout J. et al. \| NatAs \| 5-268 \| 2021 \| 2021NatAs...5..268D \| http://ui.adsabs.harvard.edu/#abs/2021NatAs...5..268D 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 Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview \|Botteon A. Shimwell T. W. et al. \| A&A \| 660-78 \| 2022 \| 2022A&A...660A..78B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan Z. S. Han J. L. \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y Linking a universal gas density profile to the core-excised X-ray luminosity in galaxy clusters up to z u223c 1.1 \|Pratt G. W. Arnaud M. et al. \| A&A \| 665-24 \| 2022 \| 2022A&A...665A..24P \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A..24P The XMM Cluster Survey: an independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies \|Turner D. J. Giles P. A. et al. \| MNRAS \| 517-657 \| 2022 \| 2022MNRAS.517..657T \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517..657T The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium \|Zhang X. Simionescu A. et al. \| A&A \| 672-42 \| 2023 \| 2023A&A...672A..42Z \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models \|Cassano R. Cuciti V. et al. \| A&A \| 672-43 \| 2023 \| 2023A&A...672A..43C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C 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 Ultra-low-frequency LOFAR spectral indices of cluster radio halos \|Pasini T. De Gasperin F. et al. \| A&A \| 689-A218 \| 2024 \| 2024A&A...689A.218P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...689A.218P Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2016-04-18T18:11:36Z/2017-01-31T21:28:38Z
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	2018-03-29T22:00:00Z
Last Update	2026-03-04
Keywords	"sample constitutes", "fundamental scalings", "etween ysz", "redshift range", "mass pea", "mass profiles", "cosmological exploitation", "M500", "resolved xray spectroscopy", "gravitational collapse", "mass population", "planck sample", "14m_sun cluster", "cluster scales"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Monique Arnaud, 2018, 'Probing the extreme mass peaks at z>0.7', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-86wsowh