A dataset provided by the European Space Agency

Name: LoCuSS: A Joint XMM-Newton Subaru Study of Galaxy Cluster Scaling Relations
Published: 2011-05-13T00:00:00Z

Proposal ID	060500
Title	LoCuSS: A Joint XMM-Newton Subaru Study of Galaxy Cluster Scaling Relations
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605000301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605000501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605000601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605000701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605000801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0605000901
DOI	https://doi.org/10.5270/esa-i0qeu2l
Principal Investigator, PI	Dr Yu-Ying Zhang
Abstract	We propose a systematic high precision investigation of the cluster massobservable scaling relations, employing XMM data and our Subaru weak lensingdata. The primary goal is to find out the best cluster mass proxy andinvestigate the behaviors of its scatter. Our preliminary results indicate thatgas mass has lower scatter with total mass, compared to the product of gas massand cluster temperature, Y_X. If those are confirmed, this will change thestrategy for carrying out the X-ray cluster cosmology. Achieving a good controlover the systematics have major implications for cluster cosmologists strivingto measure the dark energy equation of state parameter, and should add a sharpmulti-wavelength focus to investigations of the cluster physics. We require to observe 10 of 27 clusters (176ksec).
Publications	Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 536-11 \| 2011 \| 2011A&A...536A..11P \| http://ui.adsabs.harvard.edu/#abs/2011A&A...536A..11P Planck intermediate results. III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 550-129 \| 2013 \| 2013A&A...550A.129P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A.129P Planck intermediate results. V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect \|Planck Collaboration, Ade, P. A. R., et al. \| A&A \| 550-131 \| 2013 \| 2013A&A...550A.131P \| http://ui.adsabs.harvard.edu/#abs/2013A&A...550A.131P 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 Scaling Relations and X-Ray Properties of Moderate-luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton \|Connor, Thomas, Donahue, Megan, et al. \| ApJ \| 794-48 \| 2014 \| 2014ApJ...794...48C \| http://ui.adsabs.harvard.edu/#abs/2014ApJ...794...48C 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 LoCuSS: The Slow Quenching of Star Formation in Cluster Galaxies and the Need for Pre-processing \|Haines, C. P., Pereira, M. J., et al. \| ApJ \| 806-101 \| 2015 \| 2015ApJ...806..101H \| http://ui.adsabs.harvard.edu/#abs/2015ApJ...806..101H 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 The XMM Cluster Survey: the halo occupation number of BOSS galaxies in X-ray clusters \|Mehrtens, Nicola, Romer, A. Kathy, et al. \| MNRAS \| 463-1929 \| 2016 \| 2016MNRAS.463.1929M \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463.1929M A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 \|Pons, E., Watson, M. G., \| A&A \| 594-72 \| 2016 \| 2016A&A...594A..72P \| http://ui.adsabs.harvard.edu/#abs/2016A&A...594A..72P Dependence of the broad Fe Kalpha line on the physical parameters of AGN \|Liu, Zhu, Yuan, Weimin, et al. \| MNRAS \| 463-684 \| 2016 \| 2016MNRAS.463..684L \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.463..684L 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 LoCuSS: pre-processing in galaxy groups falling into massive galaxy clusters at z = 0.2 \|Bianconi, M., Smith, G. P., et al. \| MNRAS \| 473-79 \| 2018 \| 2018MNRAS.473L..79B \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.473L..79B Connecting optical and X-ray tracers of galaxy cluster relaxation \|Roberts, Ian D., Parker, Laura C., \| MNRAS \| 475-4704 \| 2018 \| 2018MNRAS.475.4704R \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.475.4704R 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 Deriving the Hubble constant using Planck and XMM-Newton observations of galaxy clusters \|Kozmanyan, Arpine, Bourdin, Herve, et al. \| A&A \| 621-34 \| 2019 \| 2019A&A...621A..34K \| http://ui.adsabs.harvard.edu/#abs/2019A&A...621A..34K 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 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 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 The Most Massive galaxy Clusters (M2C) across cosmic time: link between radial total mass distribution and dynamical state \|Bartalucci, I., Arnaud, M., et al. \| A&A \| 628-86 \| 2019 \| 2019A&A...628A..86B \| http://ui.adsabs.harvard.edu/#abs/2019A&A...628A..86B 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 On the Reliability of Photometric and Spectroscopic Tracers of Halo Relaxation \|Zhoolideh Haghighi, Mohammad H., Raouf, Mojtaba, et al. \| ApJ \| 904-36 \| 2020 \| 2020ApJ...904...36Z \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...904...36Z 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 PACT. II. Pressure profiles of galaxy clusters using Planck and ACT \|Pointecouteau, E., Santiago-Bautista, I., et al. \| A&A \| 651-73 \| 2021 \| 2021A&A...651A..73P \| http://ui.adsabs.harvard.edu/#abs/2021A&A...651A..73P The Planck clusters in the LOFAR sky. I. LoTSS-DR2: New detections and sample overview \|Botteon, A., Shimwell, T. W., et al. \| A&A \| 660-78 \| 2022 \| 2022A&A...660A..78B \| http://ui.adsabs.harvard.edu/#abs/2022A&A...660A..78B 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 Linking a universal gas density profile to the core-excised X-ray luminosity in galaxy clusters up to z \\u223c 1.1 \|Pratt, G. W., Arnaud, M., et al. \| A&A \| 665-24 \| 2022 \| 2022A&A...665A..24P \| http://ui.adsabs.harvard.edu/#abs/2022A&A...665A..24P Heating of the intracluster medium by buoyant bubbles and sound waves \|Iqbal, Asif, Majumdar, Subhabrata, et al. \| MNRAS \| 518-2735 \| 2023 \| 2023MNRAS.518.2735I \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.518.2735I 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 The Planck clusters in the LOFAR sky. III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium \|Zhang, X., Simionescu, A., et al. \| A&A \| 672-42 \| 2023 \| 2023A&A...672A..42Z \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..42Z The Planck clusters in the LOFAR sky. IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models \|Cassano, R., Cuciti, V., et al. \| A&A \| 672-43 \| 2023 \| 2023A&A...672A..43C \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..43C 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 The first evidence of tidally induced activity in a brown dwarf-M dwarf pair: a Chandra study of the NLTT 41135/41136 system \|Ili\\u0107, Nikoleta, Poppenhaeger, Katja, et al. \| MNRAS \| 524-5954 \| 2023 \| 2023MNRAS.524.5954I \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524.5954I 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 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 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	2009-06-17T06:51:27Z/2010-04-25T21:24:37Z
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	2011-05-13T00:00:00Z
Keywords	"cluster cosmologists striving", "dark energy equation", "xray cluster cosmology", "employing xmm data", "cluster mass proxy", "XMM", "lower scatter", "cluster physics", "precision investigation", "major implications", "cluster temperature", "total mass", "XMM-Newton", "cluster 176", "xmm newton subaru", "gas mass"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yu-Ying Zhang, 2011, 'LoCuSS: A Joint XMM-Newton Subaru Study of Galaxy Cluster Scaling Relations', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-i0qeu2l