A dataset provided by the European Space Agency

Name: Exploring X-ray Properties of Shear-Selected Clusters in the HSC SSP Field
Published: 2019-05-14T22:00:00Z

Proposal ID	080441
Title	Exploring X-ray Properties of Shear-Selected Clusters in the HSC SSP Field
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804410101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804410201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0804410501
DOI	https://doi.org/10.5270/esa-cjpx4es
Principal Investigator, PI	Dr Ikuyuki Mitsuishi
Abstract	The HSC SSP survey constructs an unprecedented shear-selected cluster catalogthrough weak gravitational lensing signals purely tracing dark matterdistribution. We here propose 260 ks X-ray follow-up observations of 9intermediate-redshift (z~0.3) and massive (MWL > 3 x 10^14 h^-1 Msolar )shear-selected clusters discovered in the current HSC SSP survey. By combininghigh quality weak lensing data with the X-ray observations, we aim to extractscaling relations between X-ray observables and weak-lensing mass precisely.XMM-Newton capabilities enable us to perform the first systematic X-ray studyfor shear-selected clusters in an unexplored parameter space.
Publications	The XMM Cluster Survey: an independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies \|Turner D. J. Giles P. A. et al. \| MNRAS \| 517-657 \| 2022 \| 2022MNRAS.517..657T \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.517..657T 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-04-22T06:07:56Z/2018-04-24T19:51:26Z
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	2019-05-14T22:00:00Z
Keywords	"msolar shear", "hsc ssp survey", "massive mwl", "extract scaling relations", "XMM", "xmm newton", "unexplored parameter space", "systematic xray", "xray observables", "intermediate redshift z", "XMM-Newton", "260 xray", "cluster catalog", "hsc ssp field", "exploring xray properties"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ikuyuki Mitsuishi, 2019, 'Exploring X-ray Properties of Shear-Selected Clusters in the HSC SSP Field', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-cjpx4es