A dataset provided by the European Space Agency

Name: Precision Mass-Observable Cluster Calibration with the HSC and ACTPol surveys
Published: 2017-02-19T23:00:00Z

Proposal ID	076287
Title	Precision Mass-Observable Cluster Calibration with the HSC and ACTPol surveys
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762870201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762870301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762870401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762870501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762870601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762870801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762870901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762871001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0762871101
DOI	https://doi.org/10.5270/esa-iixn9uu
Principal Investigator, PI	Dr Nobuhiro Okabe
Abstract	We propose a systematic study to calibrate how various galaxy clusterobservables scale with mass, using precision, HSC-derived, weak lensing massmeasurements and make a stringent test of the assumption of hydrostaticequilibrium of clusters. The exquisite quality of multi-band HSC imaging willenable us to improve both the precision and accuracy of weak-lensing massmeasurements, and allow us to significantly reduce systematic error forindividual cluster mass measurements. By combining these weak lensing massmeasurements wit deep XMM-Newton X-ray and ACTPol Sunyaev-Zel.dovich effectdata, we will have an unprecedented ability to constrain the physical state ofthe intracluster medium. Our project provides an essential bridge to future, cluster-based, cosmological studies by eROSITA.
Publications	X-Ray Morphological Analysis of the Planck ESZ Clusters \|Lovisari, Lorenzo, Forman, William R., et al. \| ApJ \| 846-51 \| 2017 \| 2017ApJ...846...51L \| http://ui.adsabs.harvard.edu/#abs/2017ApJ...846...51L 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 Multiwavelength study of X-ray luminous clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field \|Miyaoka, Keita, Okabe, Nobuhiro, et al. \| PASJ \| 70-22 \| 2018 \| 2018PASJ...70S..22M \| http://ui.adsabs.harvard.edu/#abs/2018PASJ...70S..22M X-ray scaling relations from a complete sample of the richest maxBCG clusters \|Ge, Chong, Sun, Ming, et al. \| MNRAS \| 484-1946 \| 2019 \| 2019MNRAS.484.1946G \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484.1946G ComPRASS: a Combined Planck-RASS catalogue of X-ray-SZ clusters \|Tarrio, P., Melin, J.-B., \| A&A \| 626-7 \| 2019 \| 2019A&A...626A...7T \| http://ui.adsabs.harvard.edu/#abs/2019A&A...626A...7T X-Ray Scaling Relations for a Representative Sample of Planck-selected Clusters Observed with XMM-Newton \|Lovisari, Lorenzo, Schellenberger, Gerrit, et al. \| ApJ \| 892-102 \| 2020 \| 2020ApJ...892..102L \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...892..102L A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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 Comparing different mass estimators for a large subsample of the Planck-ESZ clusters \|Lovisari, L., Ettori, S., et al. \| A&A \| 644-78 \| 2020 \| 2020A&A...644A..78L \| http://ui.adsabs.harvard.edu/#abs/2020A&A...644A..78L The thermalization of massive galaxy clusters \|Sereno, Mauro, Lovisari, Lorenzo, et al. \| MNRAS \| 507-5214 \| 2021 \| 2021MNRAS.507.5214S \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.5214S 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 Scaling relations of X-ray luminous clusters in the Hyper Suprime-Cam Subaru Strategic Program field \|Poon, Helen, Okabe, Nobuhiro, et al. \| MNRAS \| 520-6001 \| 2023 \| 2023MNRAS.520.6001P \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.520.6001P Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters \|Wicker, R., Douspis, M., et al. \| A&A \| 674-48 \| 2023 \| 2023A&A...674A..48W \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A..48W X\\u2011HESS: A large sample of highly accreting serendipitous AGN under the XMM\\u2011Newton microscope \|Laurenti, M., Tombesi, F., et al. \| AN \| 344-20230053 \| 2023 \| 2023AN....34430053L \| http://ui.adsabs.harvard.edu/#abs/2023AN....34430053L 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 AGNs in massive galaxy clusters: Role of galaxy merging, infalling groups, cluster mass, and dynamical state \|Koulouridis, E., Gkini, A., \| A&A \| 684-A111 \| 2024 \| 2024A&A...684A.111K \| http://ui.adsabs.harvard.edu/#abs/2024A&A...684A.111K 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	2015-06-22T18:23:06Z/2016-02-09T05:24:14Z
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	2017-02-19T23:00:00Z
Keywords	"intracluster medium", "dovich effect data", "XMM", "actpol sunyaev zel", "exquisite quality", "reduce systematic error", "XMM-Newton", "actpol surveys", "hydrostatic equilibrium", "stringent test"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Nobuhiro Okabe, 2017, 'Precision Mass-Observable Cluster Calibration with the HSC and ACTPol surveys', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-iixn9uu