A dataset provided by the European Space Agency

Name: THE X-RAY PROPERTIES OF HIGH REDSHIFT WEAK-LENSING SELECTED GALAXY CLUSTERS
Published: 2013-02-04T00:00:00Z

Proposal ID	067466
Title	THE X-RAY PROPERTIES OF HIGH REDSHIFT WEAK-LENSING SELECTED GALAXY CLUSTERS
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674660201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0674660301
DOI	https://doi.org/10.5270/esa-kj2i2z4
Principal Investigator, PI	Mr Paul Giles
Abstract	We propose XMM observations (totaling 107 ks) of 6 galaxy clusters in theredshift range 0.3 < z < 0.6 selected in a Subaru weak lensing (WL) survey. Thiswill complete a sample of 8 clusters that will be used to study systematicallythe X-ray properties of clusters detected independently of their baryoniccontent. We will investigate biases in cluster selection techniques for high-zclusters, compare the high-z scaling relations of the X-ray properties (e.g. Lx,kT, Mgas, Yx) of WL selected clusters to those of X-ray selected clusters,investigate the evolution of the properties of WL selected clusters from thelocal to high redshift universe and study their morphology/structure.
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 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 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2012-01-06T14:35:14Z/2012-01-07T00:01:23Z
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	2013-02-04T00:00:00Z
Keywords	"xray properties", "XMM", "redshift weak lensing", "redshift range", "galaxy clusters", "galaxy cluster", "z clusters", "redshift universe", "baryonic content", "cluster selection techniques", "totaling 107", "z scaling relations"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Mr Paul Giles, 2013, 'THE X-RAY PROPERTIES OF HIGH REDSHIFT WEAK-LENSING SELECTED GALAXY CLUSTERS', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-kj2i2z4