A dataset provided by the European Space Agency

Name: A new Cosmological Study Approach with a Volume Limited X-ray Cluster Sample
Published: 2013-02-16T00:00:00Z

Proposal ID	067547
Title	A new Cosmological Study Approach with a Volume Limited X-ray Cluster Sample
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DOI	https://doi.org/10.5270/esa-4jwybcu
Principal Investigator, PI	Prof Hans Boehringer
Abstract	The application of galaxy clusters in constraining cosmological models iscurrently mostly limited by our uncertain knowledge of scaling relations of easyobservables and cluster mass. Most of the scaling relation studies are based onX-ray flux limited samples. Here we propose to take a new approach to studygalaxy cluster properties in a volume-limited sample. From the comparison offlux and volume-limited samples we would be able to determine the intrinsicscatter of scaling relations in an unambiguous way, providing an importantadvance in cluster cosmology studies. Apart from the cosmological application,the volume-limited survey of nearby clusters will also provide a great benchmarksample for all aspects of characterizing the properties of the cluster population.
Publications	A volume-limited sample of X-ray galaxy groups and clusters - I. Radial entropy and cooling time profiles \|Panagoulia, E. K., Fabian, A. C., \| MNRAS \| 438-2341 \| 2014 \| 2014MNRAS.438.2341P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.438.2341P 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 KAT-7 observations of an unbiased sample of mass-selected galaxy clusters \|Bernardi, G., Venturi, T., et al. \| MNRAS \| 456-1259 \| 2016 \| 2016MNRAS.456.1259B \| http://ui.adsabs.harvard.edu/#abs/2016MNRAS.456.1259B 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 A volume-limited sample of X-ray galaxy groups and clusters - II. X-ray cavity dynamics \|Panagoulia, E. K., Fabian, A. C., et al. \| MNRAS \| 444-1236 \| 2014 \| 2014MNRAS.444.1236P \| http://ui.adsabs.harvard.edu/#abs/2014MNRAS.444.1236P 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 H I absorption in nearby compact radio galaxies \|Glowacki, M., Allison, J. R., et al. \| MNRAS \| 467-2766 \| 2017 \| 2017MNRAS.467.2766G \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.467.2766G 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 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 The non-uniformity of galaxy cluster metallicity profiles \|Lovisari, L., Reiprich, T. H., \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters \|Lagana, T. F., Durret, F., \| MNRAS \| 484-2807 \| 2019 \| 2019MNRAS.484.2807L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.484.2807L 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 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 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 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 Low-frequency integrated radio spectra of diffuse, steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP \|Duchesne, S. W., Johnston-Hollitt, M., \| PASA \| 38-53 \| 2021 \| 2021PASA...38...53D \| http://ui.adsabs.harvard.edu/#abs/2021PASA...38...53D 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 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 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 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	RGS1, EPN, RGS2, EMOS1, OM, EMOS2
Temporal Coverage	2011-04-30T18:05:12Z/2012-02-02T05:56:47Z
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	2013-02-16T00:00:00Z
Keywords	"easy observables", "uncertain knowledge", "cluster population", "volume limited survey", "cluster cosmology", "scaling relations", "constraining cosmological models", "galaxy cluster", "cosmological application", "volume limited samples", "scaling relation", "cluster mass", "volume limited sample", "nearby cluster", "galaxy cluster properties", "benchmark sample"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Hans Boehringer, 2013, 'A new Cosmological Study Approach with a Volume Limited X-ray Cluster Sample', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-4jwybcu