A dataset provided by the European Space Agency

Name: Are massive clusters always X-ray luminousquestionMark
Published: 2012-05-10T00:00:00Z

Proposal ID	065381
Title	Are massive clusters always X-ray luminous?
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653810501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0653810601
DOI	https://doi.org/10.5270/esa-w4515dj
Principal Investigator, PI	Dr Ming Sun
Abstract	Studies of galaxy clusters are important for both cosmology and the formation ofbaryonic structures. An important relation in cluster science is the f_gas - Mrelation. However, the cluster samples used to constrain this relation are X-rayselected and the current XMM and Chandra archives are also heavily biased toX-ray selected clusters. To address this important bias, we construct a sampleof 18 most massive clusters from the SDSS-C4 cluster catalog. Nine of them havebeen observed by XMM or Chandra but they are all X-ray luminous, while eight ofthe other nine unobserved clusters are X-ray faint. We propose to observe thesenine unobserved clusters to complete this unique sample, with potentiallyimportant implications on the cluster mass - proxy relations.
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 The XMM Cluster Survey: predicted overlap with the Planck Cluster Catalogue \|Viana, Pedro T. P., da Silva, Antonio, et al. \| MNRAS \| 422-1007 \| 2012 \| 2012MNRAS.422.1007V \| http://ui.adsabs.harvard.edu/#abs/2012MNRAS.422.1007V The amazing diversity in the hot gas content of an X-ray unbiased massive galaxy clusters sample \|Andreon, S., Serra, Ana Laura, et al. \| A&A \| 585-147 \| 2016 \| 2016A&A...585A.147A \| http://ui.adsabs.harvard.edu/#abs/2016A&A...585A.147A 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 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 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 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 HICOSMO - cosmology with a complete sample of galaxy clusters - I. Data analysis, sample selection and luminosity-mass scaling relation \|Schellenberger, G., Reiprich, T. H., \| MNRAS \| 469-3738 \| 2017 \| 2017MNRAS.469.3738S \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.3738S Variegate galaxy cluster gas content: Mean fraction, scatter, selection effects, and covariance with X-ray luminosity \|Andreon, S., Wang, J., et al. \| A&A \| 606-24 \| 2017 \| 2017A&A...606A..24A \| http://ui.adsabs.harvard.edu/#abs/2017A&A...606A..24A Intrinsic scatter of caustic masses and hydrostatic bias: An observational study \|Andreon, S., Trinchieri, G., et al. \| A&A \| 606-25 \| 2017 \| 2017A&A...606A..25A \| http://ui.adsabs.harvard.edu/#abs/2017A&A...606A..25A 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 Revived fossil plasma sources in galaxy clusters \|Mandal, S., Intema, H. T., et al. \| A&A \| 634-4 \| 2020 \| 2020A&A...634A...4M \| http://ui.adsabs.harvard.edu/#abs/2020A&A...634A...4M 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 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 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 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 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	2010-07-29T02:22:25Z/2011-04-23T14:47:00Z
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	2012-05-10T00:00:00Z
Keywords	"massive cluster", "SDSS", "XMM", "heavily biased", "xray luminous", "baryonic structures", "galaxy cluster", "xray faint", "chandra archives", "cluster samples", "cluster science", "xray luminous ?."
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ming Sun, 2012, 'Are massive clusters always X-ray luminousquestionMark', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-w4515dj