A dataset provided by the European Space Agency

Name: A combined X-ray and SZ study of the growth of cosmic structure
Published: 2013-04-18T00:00:00Z

Proposal ID	067501
Title	A combined X-ray and SZ study of the growth of cosmic structure
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0675010901
DOI	https://doi.org/10.5270/esa-g16634z
Principal Investigator, PI	Dr Karl Andersson
Abstract	We propose to study the growth of cosmic structure by completing X-rayobservations of the 20 z>0.7 clusters discovered in the first 600d of the SPTcluster survey. This proposal requests 545 ksec for 9 clusters with measuredredshifts 0.73x10^14 M_sun. These observations are a criticalpart of a multi-wavelength campaign to calibrate SZE selected cluster massesusing X-ray, weak lensing and velocity dispersions. In addition, the X-rayobservations will directly constrain properties of clusters at z~1, includingthe metallicity of the ICM, the cool core fraction, and the deviations fromself-similar evolution at high redshift. When combined with WMAP 7-year resultsand the SPT survey, the X-ray mass calibration will allow a 6% constraint on w, the dark energy equation of state parameter.
Publications	SPT-CL J0205-5829: A z = 1.32 Evolved Massive Galaxy Cluster in the South Pole Telescope Sunyaev-Zeldovich Effect Survey \|Stalder B. Ruel J. et al. \| ApJ \| 763-93 \| 2013 \| 2013ApJ...763...93S \| http://ui.adsabs.harvard.edu/#abs/2013ApJ...763...93S 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 Baryon content of massive galaxy clusters at 0.57 < z < 1.33 \|Chiu I. Mohr J. et al. \| MNRAS \| 455-258 \| 2016 \| 2016MNRAS.455..258C \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.455..258C 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 Cluster mass calibration at high redshift: HST weak lensing analysis of 13 distant galaxy clusters from the South Pole Telescope Sunyaev-Zeldovich Survey \|Schrabback T. Applegate D. et al. \| MNRAS \| 474-2635 \| 2018 \| 2018MNRAS.474.2635S \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.474.2635S X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 < z < 1.5 Observed with XMM-Newton \|Bulbul Esra Chiu I.-Non et al. \| ApJ \| 871-50 \| 2019 \| 2019ApJ...871...50B \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...871...50B Mass calibration of the CODEX cluster sample using SPIDERS spectroscopy - II. The X-ray luminosity-mass relation \|Capasso R. Mohr J. J. et al. \| MNRAS \| 494-2736 \| 2020 \| 2020MNRAS.494.2736C \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.2736C Constraining radio mode feedback in galaxy clusters with the cluster radio AGNs properties to z u223c 1 \|Gupta N. Pannella M. et al. \| MNRAS \| 494-1705 \| 2020 \| 2020MNRAS.494.1705G \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.494.1705G A joint SZ-X-ray-optical analysis of the dynamical state of 288 massive galaxy clusters \|Zenteno A. Hernu00e1ndez-Lang D. et al. \| MNRAS \| 495-705 \| 2020 \| 2020MNRAS.495..705Z \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.495..705Z Blasts from the Past: Supernova Shock Breakouts among X-Ray Transients in the XMM-Newton Archive \|Alp Dennis Larsson Josefin \| ApJ \| 896-39 \| 2020 \| 2020ApJ...896...39A \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...39A A Supernova Candidate at z = 0.092 in XMM-Newton Archival Data \|Novara Giovanni Esposito Paolo et al. \| ApJ \| 898-37 \| 2020 \| 2020ApJ...898...37N \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...898...37N A new multiwavelength census of blazars \|Paggi A. Bonato M. et al. \| A&A \| 641-62 \| 2020 \| 2020A&A...641A..62P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A..62P Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8 \|Ghirardini Vittorio Bulbul Esra et al. \| ApJ \| 910-14 \| 2021 \| 2021ApJ...910...14G \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...910...14G Constraints on the variation of fine structure constant from joint SPT-SZ and XMM-Newton observations \|Bora Kamal Desai Shantanu \| JCAP \| 2-12 \| 2021 \| 2021JCAP...02..012B \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...02..012B Thermodynamic evolution of the z = 1.75 galaxy cluster IDCS J1426.5+3508 \|Andreon S. Romero C. et al. \| MNRAS \| 505-5896 \| 2021 \| 2021MNRAS.505.5896A \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.505.5896A A test of cosmic distance duality relation using SPT-SZ galaxy clusters Type Ia supernovae and cosmic chronometers \|Bora Kamal Desai Shantanu \| JCAP \| 6-52 \| 2021 \| 2021JCAP...06..052B \| http://ui.adsabs.harvard.edu/#abs/2021JCAP...06..052B 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 EXTraS project: Exploring the X-ray transient and variable sky \|De Luca A. Salvaterra R. et al. \| A&A \| 650-167 \| 2021 \| 2021A&A...650A.167D \| http://ui.adsabs.harvard.edu/#abs/2021A&A...650A.167D The history of metal enrichment traced by X-ray observations of high-redshift galaxy clusters \|Flores Anthony M. Mantz Adam B. et al. \| MNRAS \| 507-5195 \| 2021 \| 2021MNRAS.507.5195F \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5195F Luminosity Function and Event Rate Density of XMM-Newton-selected Supernova Shock Breakout Candidates \|Sun Hui Liu He-Yang et al. \| ApJ \| 927-224 \| 2022 \| 2022ApJ...927..224S \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...927..224S A 600 kpc complex radio source at the center of Abell 3718 discovered by the EMU and POSSUM surveys \|Loi F. Brienza M. et al. \| A&A \| 672-28 \| 2023 \| 2023A&A...672A..28L \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..28L XMM-Newton-discovered Fast X-ray Transients: host galaxies and limits on contemporaneous detections of optical counterparts \|Eappachen D. Jonker P. G. et al. \| MNRAS \| 527-11823 \| 2024 \| 2024MNRAS.52711823E \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.52711823E 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 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	2011-06-07T19:48:58Z/2012-03-29T22:19:37Z
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	2013-04-18T00:00:00Z
Last Update	2025-01-27
Keywords	"dark energy equation", "cool core fraction", "cosmic structure", "M500", "constrain properties", "completing xray", "spt survey", "velocity dispersions", "xray mass calibration", "combined xray", "requests 545", "spt cluster survey", "weak lensing", "calibrate sze", "multi wavelength campaign", "cluster masses"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Karl Andersson, 2013, 'A combined X-ray and SZ study of the growth of cosmic structure', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-g16634z