The origin of diffuse radio sources, so-called cluster radio halos and relics isstill shrouded in mystery. The LOFAR Two-Metre Sky Survey of the 350 sq degHETDEX field is breaking new ground in the study of diffuse radio sources as itshows diffuse emission in a large fraction of the SZ-detected clusters in thatarea. In particular, it has revealed diffuse radio sources in a number oflow-mass clusters. While this field has good multi-wavelength coverage, there isrelatively little X-ray data of the clusters that host this newly discoveredemission. The aim of this proposal is to characterize the physical propertiesand the dynamical state of all Planck-detected clusters in this sample.
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
LOFAR observations of galaxy clusters in HETDEX. Extraction and self-calibration of individual LOFAR targets |van Weeren, R. J., Shimwell, T. W., et al. | A&A | 651-115 | 2021 | 2021A&A...651A.115V | http://ui.adsabs.harvard.edu/#abs/2021A&A...651A.115V
uGMRT detection of cluster radio emission in low-mass Planck Sunyaev-Zel.dovich clusters |Paul, Surajit, Gupta, Prateek, et al. | MNRAS | 506-5389 | 2021 | 2021MNRAS.506.5389P | http://ui.adsabs.harvard.edu/#abs/2021MNRAS.506.5389P
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
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
Search for interacting galaxy clusters from SDSS DR-17 employing optimized friends-of-friends algorithm and multimessenger tracers |Oak, Tejas, Paul, Surajit, | MNRAS | 528-5924 | 2024 | 2024MNRAS.528.5924O | http://ui.adsabs.harvard.edu/#abs/2024MNRAS.528.5924O
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, Prof Marcus Bruggen, 2020, 'The hidden side of galaxy clusters\\: diffuse emission in the HETDEX field', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-mt6y0a0
