A dataset provided by the European Space Agency

Name: The dark matter distribution in 0.9 &lt; z &lt; 1.1 clusters openParre-observationclosePar
Published: 2016-11-02T23:00:00Z

Proposal ID	076367
Title	The dark matter distribution in 0.9 < z < 1.1 clusters (re-observation)
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763670201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0763670301
DOI	https://doi.org/10.5270/esa-f50irc7
Principal Investigator, PI	Dr Monique Arnaud
Abstract	We have been awarded a Large Program in AO13 to measure the mass profiles of acomplete sample of massive galaxy clusters at 0.9< z< 1.15, with a precisionsimilar to that currently obtained for local objects. The primary goal is toassess the evolution of the dark matter concentration at cluster scales, acritical test of theoretical scenario of structure formation. This data set willalso constrain the evolution of fundamental mass-proxy relations and theevolution of the gas entropy and pressure profiles in the high mass regime, atest of gravitational gas heating. We propose to re-observe two targets, theobservation of which was dramatically affected by flares.
Publications	Resolving the hydrostatic mass profiles of galaxy clusters at z &tilde 1 with XMM-Newton and Chandra \|Bartalucci, I., Arnaud, M., et al. \| A&A \| 617-64 \| 2018 \| 2018A&A...617A..64B \| http://ui.adsabs.harvard.edu/#abs/2018A&A...617A..64B High density of active galactic nuclei in the outskirts of distant galaxy clusters \|Koulouridis, E., Bartalucci, I., \| A&A \| 623-10 \| 2019 \| 2019A&A...623L..10K \| http://ui.adsabs.harvard.edu/#abs/2019A&A...623L..10K The Galaxy Cluster Mass Scale and Its Impact on Cosmological Constraints from the Cluster Population \|Pratt, G. W., Arnaud, M., et al. \| SSRv \| 215-25 \| 2019 \| 2019SSRv..215...25P \| http://ui.adsabs.harvard.edu/#abs/2019SSRv..215...25P The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state \|Bartalucci, I., Arnaud, M., et al. \| A&A \| 628-86 \| 2019 \| 2019A&A...628A..86B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..86B 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 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-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	2015-05-22T00:03:39Z/2015-10-14T17:47:40Z
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	2016-11-02T23:00:00Z
Keywords	"mass regime", "cluster scales", "cluster re", "dark matter distribution", "mass profiles", "complete sample", "dark matter concentration", "gas entropy", "data set", "massive galaxy cluster", "pressure profiles", "structure formation", "gravitational gas heating", "local objects"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Monique Arnaud, 2016, 'The dark matter distribution in 0.9 < z < 1.1 clusters openParre-observationclosePar', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-f50irc7