A dataset provided by the European Space Agency

Name: XMM-Subaru:Complete High Precision Study of Galaxy Clusters for Modern Cosmology
Published: 2014-02-01T00:00:00Z

Proposal ID	069301
Title	XMM-Subaru:Complete High Precision Study of Galaxy Clusters for Modern Cosmology
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693010101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693010201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693010301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693010401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693010501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693010601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693010801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693011001 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0693011301
DOI	https://doi.org/10.5270/esa-g8ruk9x
Principal Investigator, PI	Dr Yu-Ying Zhang
Abstract	We request 382 ks data for 12 clusters to complete our survey of avolume-limited sample of 55 clusters. We investigated the existing data, whichhints a mass dependent bias in the X-ray to weak lensing mass ratios fordisturbed ones. X-ray mass proxies, e.g., Yx, show low scatter, but the bestfits, particularly the slopes, of the mass-observable relations may be biaseddue to this mass dependence. Our program will quantify any mass/radial dependentbias based on three independent probes (X-ray/lensing/velocity dispersion) forsuch a volume-limited sample, and deliver definitive constraints on systematicsfor upcoming cluster cosmology surveys. The dataset will be a major asset forprograms aiming to measure dark energy and programs adding a multi-wavelength focus to studies of cluster physics.
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 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 Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function \|Vagnetti, F., Middei, R., et al. \| A&A \| 593-55 \| 2016 \| 2016A&A...593A..55V \| http://ui.adsabs.harvard.edu/#abs/2016A&A...593A..55V 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 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 An off-axis galaxy cluster merger: Abell 0141 \|Caglar, Turgay, \| MNRAS \| 475-2870 \| 2018 \| 2018MNRAS.475.2870C \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.2870C 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 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 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 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 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 Imaging results from the legacy Giant Metrewave Radio Telescope Galaxy Cluster Key Project \|George, Lijo T., Kale, Ruta, \| MNRAS \| 507-4487 \| 2021 \| 2021MNRAS.507.4487G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.4487G A Multiwavelength Dynamical State Analysis of ACT-CL J0019.6+0336 \|Pillay, Denisha S., Turner, David J., et al. \| Galax \| 9-97 \| 2021 \| 2021Galax...9...97P \| http://ui.adsabs.harvard.edu/#abs/2021Galax...9...97P Tidal star-planet interaction and its observed impact on stellar activity in planet-hosting wide binary systems \|Ilic, N., Poppenhaeger, K., \| MNRAS \| 513-4380 \| 2022 \| 2022MNRAS.513.4380I \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.4380I 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 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 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 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 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 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	2012-05-27T22:27:26Z/2013-01-01T22:04:46Z
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	2014-02-01T00:00:00Z
Keywords	"probes xray", "deliver definitive constraints", ".", "mass observable relations", "mass dependent bias", "radial dependent bias", "multi wavelength focus", "modern cosmology", " yx", "382 data", "velocity dispersion", "volume limited sample", "programs aiming", "XMM", "cluster physics", "cluster cosmology surveys", "dark energy", "major asset", "xray mass proxies", "galaxy cluster", "existing data", "low scatter", "xmm subaru"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yu-Ying Zhang, 2014, 'XMM-Subaru:Complete High Precision Study of Galaxy Clusters for Modern Cosmology', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-g8ruk9x