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
Last Update	2025-01-27
Keywords	"XMM", "massive mwl", "cluster catalog", "exploring xray properties", "xmm newton", "hsc ssp field", "XMM-Newton", "unexplored parameter space", "systematic xray", "hsc ssp survey", "260 xray", "extract scaling relations", "msolar shear", "xray observables", "intermediate redshift z"
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