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-Zel.dovich 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 today.s clusters; (iv) resolve the major uncertainties inmass determinations that limit cosmological inferences; (v) build the foundationfor cluster science with next-generation surveys.
Publications
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
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
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
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
AGNs in massive galaxy clusters: Role of galaxy merging, infalling groups, cluster mass, and dynamical state |Koulouridis, E., Gkini, A., | A&A | 684-A111 | 2024 | 2024A&A...684A.111K | http://ui.adsabs.harvard.edu/#abs/2024A&A...684A.111K
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
2019-04-18T08:24:56Z/2020-08-30T23:18:20Z
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.
European Space Agency, Dr M S Arnaud-Ettori, 2020, 'Witnessing the culmination of structure formation in the Universe', 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-4m1ej30
