A dataset provided by the European Space Agency

Name: LoCuSS: completing a volume limited sample of massive clusters with XMM-Subaru
Published: 2011-07-22T00:00:00Z

Proposal ID	065201
Title	LoCuSS: completing a volume limited sample of massive clusters with XMM-Subaru
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652010101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652010201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652010301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0652010401
DOI	https://doi.org/10.5270/esa-8t5cwzw
Principal Investigator, PI	Dr Yu-Ying Zhang
Abstract	An XMM/Subaru study of 12 clusters shows that Mgas is an excellent mass proxy,with its scatter <3+/-6%. However the X-ray to weak lensing mass ratio ismorphology dependent, and sensitive to inclusion/exclusion of individualclusters. A complete volume limited sample of 54 clusters with high qualityX-ray and weak-lensing data will deliver the definitive constraints on mass biaswith respect to morphology that are essential for proper control of systematicsin forthcoming X-ray cluster cosmology programs aiming to measure the darkenergy equation of state parameter w, and for any program wishing to add a sharpmulti-wavelength focus to investigations of cluster physics. Archival data existfor 50/54 clusters; we request totaling 110 net ks for 4 clusters.
Publications	The Extended GMRT Radio Halo Survey. I. New upper limits on radio halos and mini-halos \|Kale, R., Venturi, T., et al. \| A&A \| 557-99 \| 2013 \| 2013A&A...557A..99K \| http://ui.adsabs.harvard.edu/#abs/2013A&A...557A..99K LoCuSS: hydrostatic mass measurements of the high-LX cluster sample - cross-calibration of Chandra and XMM-Newton \|Martino, Rossella, Mazzotta, Pasquale, et al. \| MNRAS \| 443-2342 \| 2014 \| 2014MNRAS.443.2342M \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.443.2342M 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 Extended GMRT Radio Halo Survey. II. Further results and analysis of the full sample \|Kale, R., Venturi, T., et al. \| A&A \| 579-92 \| 2015 \| 2015A&A...579A..92K \| http://ui.adsabs.harvard.edu/#abs/2015A&A...579A..92K 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 Brightest cluster galaxies in the extended GMRT radio halo cluster sample. Radio properties and cluster dynamics \|Kale, R., Venturi, T., et al. \| A&A \| 581-23 \| 2015 \| 2015A&A...581A..23K \| http://ui.adsabs.harvard.edu/#abs/2015A&A...581A..23K 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 AGN spectral states from simultaneous UV and X-ray observations by XMM-Newton \|Svoboda, J., Guainazzi, M., \| A&A \| 603-127 \| 2017 \| 2017A&A...603A.127S \| http://ui.adsabs.harvard.edu/#abs/2017A&A...603A.127S On the Connection between Turbulent Motions and Particle Acceleration in Galaxy Clusters \|Eckert, D., Gaspari, M., et al. \| ApJ \| 843-29 \| 2017 \| 2017ApJ...843L..29E \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...843L..29E New giant radio sources and underluminous radio halos in two galaxy clusters \|Cuciti, V., Brunetti, G., et al. \| A&A \| 609-61 \| 2018 \| 2018A&A...609A..61C \| http://ui.adsabs.harvard.edu/#abs/2018A&A...609A..61C LoCuSS: The infall of X-ray groups on to massive clusters \|Haines, C. P., Finoguenov, A., et al. \| MNRAS \| 477-4931 \| 2018 \| 2018MNRAS.477.4931H \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.477.4931H 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 LoCuSS: scaling relations between galaxy cluster mass, gas, and stellar content \|Mulroy, Sarah L., Farahi, Arya, et al. \| MNRAS \| 484-60 \| 2019 \| 2019MNRAS.484...60M \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484...60M Detection of anti-correlation of hot and cold baryons in galaxy clusters \|Farahi, Arya, Mulroy, Sarah L., et al. \| NatCo \| 10-2504 \| 2019 \| 2019NatCo..10.2504F \| http://ui.adsabs.harvard.edu/#abs/2019NatCo..10.2504F Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX-T scaling relation \|Migkas, K., Schellenberger, G., et al. \| A&A \| 636-15 \| 2020 \| 2020A&A...636A..15M \| http://ui.adsabs.harvard.edu/#abs/2020A&A...636A..15M The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava, S., Giles, P. A., et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B 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 Cosmological implications of the anisotropy of ten galaxy cluster scaling relations \|Migkas, K., Pacaud, F., et al. \| A&A \| 649-151 \| 2021 \| 2021A&A...649A.151M \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A.151M Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan, Z. S., Han, J. L., \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y The alignment between brightest cluster galaxies and host clusters \|Yuan, Z. S., Wen, Z. L., \| MNRAS \| 516-3159 \| 2022 \| 2022MNRAS.516.3159Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.516.3159Y More relaxed intracluster gas than galaxies in clusters in quasi-equilibrium \|Yuan, Z. S., Han, J. L., et al. \| MNRAS \| 523-1364 \| 2023 \| 2023MNRAS.523.1364Y \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.523.1364Y The effect of cluster dynamical state on ram-pressure stripping \|Louren\\u00e7o, Ana C. C., Jaff\\u00e9, Y. L., et al. \| MNRAS \| 526-4831 \| 2023 \| 2023MNRAS.526.4831L \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.526.4831L 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 Distribution of Merging and Post-merger Galaxies in Nearby Galaxy Clusters \|Kim, Duho, Sheen, Yun-Kyeong, et al. \| ApJ \| 966-124 \| 2024 \| 2024ApJ...966..124K \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...966..124K 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	2010-05-13T06:46:54Z/2010-07-04T09:50:45Z
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	2011-07-22T00:00:00Z
Keywords	"dark energy equation", "massive cluster", "XMM", "archival data exist", "cluster physics", "quality xray", "definitive constraints", "totaling 110", "mass proxy", "mass bias", "weak lensing data", "program wishing", "individual clusters", "proper control", "volume limited sample", "xmm subaru", "morphology dependent"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yu-Ying Zhang, 2011, 'LoCuSS: completing a volume limited sample of massive clusters with XMM-Subaru', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-8t5cwzw