A dataset provided by the European Space Agency

Name: Witnessing the culmination of structure formation in the Universe
Published: 2021-02-02T00:00:00Z

Proposal ID	082731
Title	Witnessing the culmination of structure formation in the Universe
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827310101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827310701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827311201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0827311401
DOI	https://doi.org/10.5270/esa-wojjj9w
Principal Investigator, PI	Dr M S Arnaud-Ettori
Abstract	This is a Heritage program to study the ultimate products of structure formationin mass and time\: a large, unbiased, signal-to-noise limited sample of galaxyclusters detected by Planck via their Sunyaev-Zeldovich effect. Completing thehigh-fidelity XMM coverage of this sample has extraordinary legacy value. Wewill (i) obtain an unbiased vision of the statistical properties of the clusterpopulation; (ii) uncover the provenance of non-gravitational heating; (iii)measure how their gas is shaped by the collapse into dark matter haloes and themergers that built todays clusters; (iv) resolve the major uncertainties in massdeterminations that limit cosmological inferences; (v) build the foundation forcluster science with next-generation surveys.
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 CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles \|Iqbal, A., Pratt, G. W., et al. \| A&A \| 679-51 \| 2023 \| 2023A&A...679A..51I \| http://ui.adsabs.harvard.edu/#abs/2023A&A...679A..51I 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 CHEX-MATE: Robust reconstruction of temperature profiles in galaxy clusters with XMM-Newton \|Rossetti, M., Eckert, D., et al. \| A&A \| 686-A68 \| 2024 \| 2024A&A...686A..68R \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A..68R CHEX-MATE: CLUster Multi-Probes in Three Dimensions (CLUMP-3D). I. Gas analysis method using X-ray and Sunyaev-Zel.dovich effect data \|Kim, Junhan, Sayers, Jack, et al. \| A&A \| 686-A97 \| 2024 \| 2024A&A...686A..97K \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A..97K
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2019-02-17T05:06:52Z/2021-01-21T14:19:34Z
Version	18.02_20200221_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	2021-02-02T00:00:00Z
Keywords	"statistical properties", "dark matter haloes", "noise limited sample", "gravitational heating", "cluster science", "major uncertainties", "built todays clusters", "fidelity xmm coverage", "iv resolve", "cluster population", "limit cosmological inferences", "XMM", "generation surveys", "planck via", "ii uncover", "unbiased vision", "time \:", "heritage program", "galaxy cluster", "sunyaev zeldovich effect", "structure formation", "mass determinations"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr M S Arnaud-Ettori, 2021, 'Witnessing the culmination of structure formation in the Universe', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-wojjj9w