A dataset provided by the European Space Agency

Name: Radio source ageing and the quenching of cooling cores in clusters
Published: 2008-05-09T00:00:00Z

Proposal ID	040663
Title	Radio source ageing and the quenching of cooling cores in clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406630201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0406630501
DOI	https://doi.org/10.5270/esa-uw3c2ua
Principal Investigator, PI	Dr Elena Belsole
Abstract	We propose to complete the high-quality X-ray observations of a sample of 35intermediate-redshift bright galaxy clusters by observing 4 with XMM-Newton. Thesample is unbiased in X-ray morphology and radio-source content, and is ofsufficient size to permit us to address the extent to which cooling flows arehalted by mechanical energy injected by radio sources, and if the dynamicalstate of the cluster gas correlates with the radio environment. This will beachieved by comparing the X-ray-derived temperature, entropy and pressurestructures with the energy contents, ages and distributions of the radio-sourcecomponents within the clusters.
Publications	The Origin of the Hot Gas in the Galactic Halo: Confronting Models with XMM-Newton Observations \|Henley, David B., Shelton, Robin L., et al. \| ApJ \| 723-935 \| 2010 \| 2010ApJ...723..935H \| http://ui.adsabs.harvard.edu/#abs/2010ApJ...723..935H An XMM-Newton Survey of the Soft X-ray Background. I. The O VII and O VIII Lines Between l = 120 and l = 240 \|Henley, David B., Shelton, Robin L., \| ApJS \| 187-388 \| 2010 \| 2010ApJS..187..388H \| http://ui.adsabs.harvard.edu/#abs/2010ApJS..187..388H A serendipitous XMM survey of the SDSS: the evolution of the colour-magnitude diagram of X-ray AGN from z= 0.8 to 0.1 \|Georgakakis, Antonis, Nandra, K., \| MNRAS \| 414-992 \| 2011 \| 2011MNRAS.414..992G \| http://ui.adsabs.harvard.edu/#abs/2011MNRAS.414..992G Exospheric solar wind charge exchange as seen by XMM-Newton \|Carter, J. A., Semba, S., \| AN \| 333-313 \| 2012 \| 2012AN....333..313C \| http://ui.adsabs.harvard.edu/#abs/2012AN....333..313C The cosmological analysis of X-ray cluster surveys - II. Application of the CR-HR method to the XMM archive \|Clerc, N., Sadibekova, T., et al. \| MNRAS \| 423-3561 \| 2012 \| 2012MNRAS.423.3561C \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.423.3561C An XMM-Newton Survey of the Soft X-Ray Background. II. An All-Sky Catalog of Diffuse O VII and O VIII Emission Intensities \|Henley, David B., Shelton, Robin L., \| ApJS \| 202-14 \| 2012 \| 2012ApJS..202...14H \| http://ui.adsabs.harvard.edu/#abs/2012ApJS..202...14H Joint Analysis of Cluster Observations. II. Chandra/XMM-Newton X-Ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies \|Mahdavi, Andisheh, Hoekstra, Henk, et al. \| ApJ \| 767-116 \| 2013 \| 2013ApJ...767..116M \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...767..116M An XMM-Newton Survey of the Soft X-Ray Background. III. The Galactic Halo X-Ray Emission \|Henley, David B., Shelton, Robin L., \| ApJ \| 773-92 \| 2013 \| 2013ApJ...773...92H \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...773...92H Probing of the Interactions between the Hot Plasmas and Galaxies in Clusters from z = 0.1 to 0.9 \|Gu, Liyi, Gandhi, Poshak, et al. \| ApJ \| 767-157 \| 2013 \| 2013ApJ...767..157G \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...767..157G Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift \|Yershov, V. N., \| Ap&SS \| 354-97 \| 2014 \| 2014Ap&SS.354...97Y \| http://ui.adsabs.harvard.edu/#abs/2014Ap&SS.354...97Y The Origin of the Hot Gas in the Galactic Halo: Testing Galactic Fountain Models. X-Ray Emission \|Henley, David B., Shelton, Robin L., et al. \| ApJ \| 800-102 \| 2015 \| 2015ApJ...800..102H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...800..102H Obscuration-dependent Evolution of Active Galactic Nuclei \|Buchner, Johannes, Georgakakis, Antonis, et al. \| ApJ \| 802-89 \| 2015 \| 2015ApJ...802...89B \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...802...89B XMM-Newton publication statistics \|Ness, J.-U., Parmar, A. N., et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Tight Relation between X-Ray and Ultraviolet Luminosity of Quasars \|Lusso, E., Risaliti, G., \| ApJ \| 819-154 \| 2016 \| 2016ApJ...819..154L \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...819..154L Erratum: Joint Analysis of Cluster Observations. II. Chandra/XMM-Newton X-Ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies (2013, ApJ, 767, 116) \|Mahdavi, Andisheh, Hoekstra, Henk, et al. \| ApJ \| 794-175 \| 2014 \| 2014ApJ...794..175M \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...794..175M The Interaction of the Fermi Bubbles with the Milky Way.s Hot Gas Halo \|Miller, Matthew J., Bregman, Joel N., \| ApJ \| 829-9 \| 2016 \| 2016ApJ...829....9M \| http://ui.adsabs.harvard.edu/#abs/2016ApJ...829....9M SPIDERS: the spectroscopic follow-up of X-ray selected clusters of galaxies in SDSS-IV \|Clerc, N., Merloni, A., et al. \| MNRAS \| 463-4490 \| 2016 \| 2016MNRAS.463.4490C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.4490C The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch, Eric W., \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Imaging Plasma Density Structures in the Soft X-Rays Generated by Solar Wind Charge Exchange with Neutrals \|Sibeck, David G., Allen, R., et al. \| SSRv \| 214-79 \| 2018 \| 2018SSRv..214...79S \| http://ui.adsabs.harvard.edu/#abs/2018SSRv..214...79S Probing the dynamical state, baryon content, and multiphase nature of galaxy clusters with bright background QSOs \|Ge, Chong, Wang, Q. Daniel, et al. \| MNRAS \| 481-4111 \| 2018 \| 2018MNRAS.481.4111G \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.481.4111G A massive cluster at z = 0.288 caught in the process of formation: The case of Abell 959 \|Birzan, L., Rafferty, D. A., et al. \| MNRAS \| 487-4775 \| 2019 \| 2019MNRAS.487.4775B \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.4775B X-ray properties of the X-CLASS-redMaPPer galaxy cluster sample: the luminosity-temperature relation \|Molham, Mona, Clerc, Nicolas, et al. \| MNRAS \| 494-161 \| 2020 \| 2020MNRAS.494..161M \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494..161M Multiwavelength classification of X-ray selected galaxy cluster candidates using convolutional neural networks \|Kosiba, Matej, Lieu, Maggie, et al. \| MNRAS \| 496-4141 \| 2020 \| 2020MNRAS.496.4141K \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.496.4141K SPIDERS: overview of the X-ray galaxy cluster follow-up and the final spectroscopic data release \|Clerc, N., Kirkpatrick, C. C., et al. \| MNRAS \| 497-3976 \| 2020 \| 2020MNRAS.497.3976C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497.3976C Constraining the Milky Way Mass with Its Hot Gaseous Halo \|Guo, Fulai, Zhang, Ruiyu, \| ApJ \| 904-14 \| 2020 \| 2020ApJ...904L..14G \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904L..14G An X-Ray- and SZ-bright Diffuse Source toward M31: A Local Hot Bridge \|Qu, Zhijie, Huang, Rui, et al. \| ApJ \| 907-14 \| 2021 \| 2021ApJ...907...14Q \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...907...14Q A Luminous X-Ray Transient in SDSS J143359.16+400636.0: A Likely Tidal Disruption Event \|Brightman, Murray, Ward, Charlotte, et al. \| ApJ \| 909-102 \| 2021 \| 2021ApJ...909..102B \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...909..102B The composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou, Min-Hua, Gu, Min-Feng, \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z Classification of 4XMM-DR9 sources by machine learning \|Zhang, Yanxia, Zhao, Yongheng, \| MNRAS \| 503-5263 \| 2021 \| 2021MNRAS.503.5263Z \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.503.5263Z 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 Solar Cycle Temporal Variation of the Solar Wind Charge Exchange X-Ray Lines \|Qu, Zhijie, Koutroumpa, Dimitra, et al. \| ApJ \| 930-21 \| 2022 \| 2022ApJ...930...21Q \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...930...21Q X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z = 6.56 \|Wolf, J., Nandra, K., et al. \| A&A \| 669-127 \| 2023 \| 2023A&A...669A.127W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...669A.127W A Multiwavelength Study of Active Galactic Nuclei in Post-merger Remnants \|Li, Wenhao, Nair, Preethi, et al. \| ApJ \| 944-168 \| 2023 \| 2023ApJ...944..168L \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...944..168L 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 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 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	2007-04-12T12:14:39Z/2007-04-13T02:02:32Z
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	2008-05-09T00:00:00Z
Keywords	"pressure structures", "radio source components", "XMM", "radio source ageing", "radio sources", "radio source content", "energy contents", "xray morphology", "quality xray", "cluster gas correlates", "cooling cores", "XMM-Newton", "cooling flows", "mechanical energy injected", "xmm newton"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Elena Belsole, 2008, 'Radio source ageing and the quenching of cooling cores in clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-uw3c2ua