A dataset provided by the European Space Agency

Name: Properties of newly-discovered low X-ray surface brightness Planck SZ clusters
Published: 2013-05-10T00:00:00Z

Proposal ID	067438
Title	Properties of newly-discovered low X-ray surface brightness Planck SZ clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674380101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674380201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674380301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674380501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674380701
DOI	https://doi.org/10.5270/esa-iqnudiq
Principal Investigator, PI	Dr Gabriel Pratt
Abstract	We wish to re-observe 8 high SNR Planck all-sky survey-discovered clusters at0.1<z<0.5. Existing XMM 10 ks snapshot observations of variable quality, carriedout as part of Planck catalogue validation, suggest that they are all hot (kT >5 keV), high mass objects with complex morphologies and density profiles farshallower than those of X-ray-selected cluster samples in the same mass range.We will measure density, temperature, entropy and pressure profiles and comparewith reference local and distant data from X-ray-selected samples. Deep X-rayobservations of these extreme objects will allow us to precisely quantify howthese new SZ-selected clusters differ from X-ray selected clusters, and assesstheir impact on mass scaling relations and X-ray and SZ selection functions.
Publications	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 Occurrence of radio halos in galaxy clusters. Insight from a mass-selected sample \|Cuciti, V., Cassano, R., et al. \| A&A \| 580-97 \| 2015 \| 2015A&A...580A..97C \| http://ui.adsabs.harvard.edu/#abs/2015A&A...580A..97C The population of X-ray supernova remnants in the Large Magellanic Cloud \|Maggi, P., Haberl, F., et al. \| A&A \| 585-162 \| 2016 \| 2016A&A...585A.162M \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.162M KAT-7 observations of an unbiased sample of mass-selected galaxy clusters \|Bernardi, G., Venturi, T., et al. \| MNRAS \| 456-1259 \| 2016 \| 2016MNRAS.456.1259B \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.456.1259B 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 Identification of high-mass X-ray binaries selected from XMM-Newton observations of the LMC* \|van Jaarsveld, N., Buckley, D. A. H., et al. \| MNRAS \| 475-3253 \| 2018 \| 2018MNRAS.475.3253V \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.3253V X-Ray Luminosity and Size Relationship of Supernova Remnants in the LMC \|Ou, Po-Sheng, Chu, You-Hua, et al. \| ApJ \| 863-137 \| 2018 \| 2018ApJ...863..137O \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...863..137O The cool-core state of Planck SZ-selected clusters versus X-ray-selected samples: evidence for cool-core bias \|Rossetti, M., Gastaldello, F., et al. \| MNRAS \| 468-1917 \| 2017 \| 2017MNRAS.468.1917R \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.468.1917R Two merging galaxy clusters with very hot shock fronts observed shortly before pericentric passage \|Lagana, T. F., Souza, G. S., et al. \| MNRAS \| 487-3922 \| 2019 \| 2019MNRAS.487.3922L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487.3922L Mass variance from archival X-ray properties of Dark Energy Survey Year-1 galaxy clusters \|Farahi, A., Chen, X., et al. \| MNRAS \| 490-3341 \| 2019 \| 2019MNRAS.490.3341F \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.490.3341F New optically identified supernova remnants in the Large Magellanic Cloud \|Yew, Miranda, Filipovi\\u0107, Miroslav D., et al. \| MNRAS \| 500-2336 \| 2021 \| 2021MNRAS.500.2336Y \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.500.2336Y 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 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 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 CHEX-MATE: Pressure profiles of six galaxy clusters as seen by SPT and Planck \|Oppizzi, F., De Luca, F., et al. \| A&A \| 672-156 \| 2023 \| 2023A&A...672A.156O \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A.156O 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 CHEX-MATE: A non-parametric deep learning technique to deproject and deconvolve galaxy cluster X-ray temperature profiles \|Iqbal, A., Pratt, G. W., et al. \| A&A \| 679-51 \| 2023 \| 2023A&A...679A..51I \| http://ui.adsabs.harvard.edu/#abs/2023A&A...679A..51I 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 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 CHEX-MATE: Robust reconstruction of temperature profiles in galaxy clusters with XMM-Newton \|Rossetti, M., Eckert, D., et al. \| A&A \| 686-A68 \| 2024 \| 2024A&A...686A..68R \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A..68R 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	2011-05-12T11:49:46Z/2012-04-20T05:59:04Z
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	2013-05-10T00:00:00Z
Keywords	"mass objects", "existing xmm", "supernova remnant planck", "precisely quantify", "XMM", "distant data", "density profiles", "planck catalogue validation", "complex morphologies", "reference local", "variable quality", "pressure profiles", "mass range", "hot kt", "sz selection functions", "deep xray", "mass scaling relations", "sky survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Gabriel Pratt, 2013, 'Properties of newly-discovered low X-ray surface brightness Planck SZ clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-iqnudiq