A dataset provided by the European Space Agency

Name: Are we missing the X-ray under-luminous clusters
Published: 2020-03-13T23:00:00Z

Proposal ID	082181
Title	Are we missing the X-ray under-luminous clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821810401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821810501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821810701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821810801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821810901
DOI	https://doi.org/10.5270/esa-rqc1bpg
Principal Investigator, PI	Dr Gerrit Schellenberger
Abstract	We propose to observe a Planck SZ selected, complete sample of 15 X-ray under-luminous galaxy clusters with XMM-Newton. This largely unstudied population ofgalaxy clusters has important consequences for cosmology. Moreover, since theunder-luminous clusters are expected to be undergoing major mergers, this sampleprovides a great opportunity to quantify energy re-distribution among thermaland non-thermal particles, study heat transport and enrichment evo- lution. Werequest 175ks of XMM-Newton time to cover the 11 clusters which lackgood-quality observations. With these data, we will determine their dynamicalstate and history, examine the processes responsible for gas heating, andmeasure the impact of such powerful mergers on cosmological studies.
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 Unusually Weak and Exceptionally Steep Radio Relic in A2108 \|Schellenberger Gerrit Giacintucci Simona et al. \| ApJ \| 925-91 \| 2022 \| 2022ApJ...925...91S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...925...91S 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 Galaksi Ku00fcmelerinde Ku00fcme u0130u00e7i Gazu0131n X-Iu015fu0131n u00d6zelliklerinin u0130ncelenmesi ile Ku00fcmelerin Dinamiksel Durumunu Belirleme ve Su0131nu0131flandu0131rma \|Yapucu Zahide Ikis Gu00fcn Gu00fclnur \| TJAA \| 4-237 \| 2023 \| 2023TJAA....4S.237Z \| http://ui.adsabs.harvard.edu/#abs/2023TJAA....4S.237Z 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 A New Enigmatic Radio Relic in the Low-mass Cluster Abell 2108 \|Chatterjee Swarna Rahaman Majidul et al. \| MNRAS \| 527-10986 \| 2024 \| 2024MNRAS.52710986C \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.52710986C 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-06-15T19:37:30Z/2019-02-19T12:13:11Z
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	2020-03-13T23:00:00Z
Last Update	2025-01-27
Keywords	"luminous clusters", "planck sz", "complete sample", "gas heating", "xmm newton", "luminous galaxy cluster", "XMM-Newton", "heat transport", "xmm newton time", "unstudied population", "powerful mergers", "galaxy cluster", "luminous cluster", "nonthermal particles", "XMM", "major mergers", "enrichment evo lution"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gerrit Schellenberger, 2020, 'Are we missing the X-ray under-luminous clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-rqc1bpg