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<z<0.9. Using for the first time a statistically significant sample in thisregime, we will extend our study of the pressure, entropy and mass profiles,their dispersion, and the fundamental scalings between etween YSZ, YX and M500,of this extreme-mass population back to a time when the Universe was 46 per centof its present age. The sample constitutes an important probe of the physics ofgravitational collapse on cluster scales, and will be of large legacy value forthe cosmological exploitation of the Planck sample.
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
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
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
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
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.
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
