A dataset provided by the European Space Agency

Name: Systematic X-ray study of distant massive clusters discovered by the HSC survey
Published: 2019-01-19T23:00:00Z

Proposal ID	080040
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=0800400101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800400201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800400301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800400401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800400501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800400601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0800400901
DOI	https://doi.org/10.5270/esa-6go7m3t
Principal Investigator, PI	Prof Naomi Ota
Abstract	We propose XMM observations of nine massive clusters of galaxies at 0.8<z<1.1newly discovered by the Subaru HSC survey, aiming at studying scaling relationsand ICM thermal evolution at high redshifts. Since distant, massive clusters arerare, the abundance of such clusters is sensitive to cosmological parameters.With a total exposure of 264 ks, we can accurately determine the ICMtemperatures and luminosities and investigate the gas profiles within r_500.This enables a systematic multi-wavelength study of the uniform sample ofoptically-selected clusters based on our X-ray, SZE, optical and weak lensingmeasurements, which will have an impact on the forthcoming cosmological studyusing clusters. Owing to its large effective area, XMM is the most suited for this study.
Publications	A new multiwavelength census of blazars \|Paggi, A., Bonato, M., et al. \| A&A \| 641-62 \| 2020 \| 2020A&A...641A..62P \| http://ui.adsabs.harvard.edu/#abs/2020A&A...641A..62P 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 ESASky SSOSS: Solar System Object Search Service and the case of Psyche \|Racero, E., Giordano, F., et al. \| A&A \| 659-38 \| 2022 \| 2022A&A...659A..38R \| http://ui.adsabs.harvard.edu/#abs/2022A&A...659A..38R 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 first evidence of tidally induced activity in a brown dwarf-M dwarf pair: a Chandra study of the NLTT 41135/41136 system \|Ili\\u0107, Nikoleta, Poppenhaeger, Katja, et al. \| MNRAS \| 524-5954 \| 2023 \| 2023MNRAS.524.5954I \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.524.5954I 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	2017-04-17T05:07:51Z/2018-01-09T20:37:45Z
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	2019-01-19T23:00:00Z
Keywords	"distant massive cluster", "massive cluster", "XMM", "uniform sample", "systematic multi wavelength", "scaling relations", "forthcoming cosmological", "cosmological parameters", "hsc survey", "gas profiles", "subaru hsc survey", "icm thermal evolution", "systematic xray", "icm temperatures", "total exposure", "weak lensing measurements"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Naomi Ota, 2019, '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-6go7m3t