A dataset provided by the European Space Agency

Name: Probing the extreme mass peaks at z>0.7
Published: 2018-03-29T22:00:00Z
License: https://creativecommons.org/licenses/by-nc/3.0/igo

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	21.51_20241115_1113
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	2026-07-09
Keywords	"resolved xray spectroscopy", "fundamental scalings", "planck sample", "mass profiles", "sample constitutes", "redshift range", "etween ysz", "14m_sun cluster", "gravitational collapse", "mass pea", "cosmological exploitation", "cluster scales", "M500", "mass population"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Monique Arnaud, 2018, 'Probing the extreme mass peaks at z>0.7', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-86wsowh
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.