A dataset provided by the European Space Agency

Name: The hidden side of galaxy clusters: diffuse emission in the HETDEX field
Published: 2020-01-17T23:00:00Z

Proposal ID	082104
Title	The hidden side of galaxy clusters: diffuse emission in the HETDEX field
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821040101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821040201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821040301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821040401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821040601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821041001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821041401
DOI	https://doi.org/10.5270/esa-mt6y0a0
Principal Investigator, PI	Prof Marcus Bruggen
Abstract	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-Zeldovich 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 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 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 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: Turbulence in the intra-cluster medium from X-ray surface brightness fluctuations \|Dupourquu00e9 S. Clerc N. et al. \| A&A \| 687-A58 \| 2024 \| 2024A&A...687A..58D \| http://ui.adsabs.harvard.edu/#abs/2024A&A...687A..58D Ultra-low-frequency LOFAR spectral indices of cluster radio halos \|Pasini T. De Gasperin F. et al. \| A&A \| 689-A218 \| 2024 \| 2024A&A...689A.218P \| http://ui.adsabs.harvard.edu/#abs/2024A&A...689A.218P Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-07-06T17:45:53Z/2018-12-17T11:51:08Z
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	2020-01-17T23:00:00Z
Last Update	2025-08-04
Keywords	"physical properties", "hetdex field", "metre sky survey", "multi wavelength coverage", "diffuse radio sources", "diffuse emission", "low mass clusters"
Publisher And Registrant	European Space Agency
Credit Guidelines	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