A dataset provided by the European Space Agency

Name: Systematic X-ray study of distant massive clusters discovered by the HSC survey
Published: 2020-03-28T23:00:00Z

Proposal ID	082129
Title	Systematic X-ray study of distant massive clusters discovered by the HSC survey
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821290201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821290401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821290501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821290601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821290801
DOI	https://doi.org/10.5270/esa-fuokzin
Principal Investigator, PI	Prof Naomi Ota
Abstract	We propose XMM observations of massive galaxies clusters at 0.8
Publications	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 Search for Young Stellar Objects within 4XMM-DR13 Using CatBoost and SPE \|Ma Xiangyao Zhang Yanxia et al. \| AJ \| 168-210 \| 2024 \| 2024AJ....168..210M \| http://ui.adsabs.harvard.edu/#abs/2024AJ....168..210M
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-05-05T03:23:20Z/2019-02-13T21:49:29Z
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	2020-03-28T23:00:00Z
Last Update	2025-08-04
Keywords	"XMM", "icm thermal evolution", "massive galaxy cluster", "distant massive cluster", "icm temperatures", "gas profiles", "massive cluster", "systematic xray", "uniform sample", "cosmological parameters", "forthcoming cosmological", "systematic multi wavelength", "cluster abundance", "targets affected", "scaling relations", "complete sample", "hsc survey", "subaru hsc survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Naomi Ota, 2020, 'Systematic X-ray study of distant massive clusters discovered by the HSC survey', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-fuokzin