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
License: https://creativecommons.org/licenses/by-nc/3.0/igo

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
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 Dynamical state of galaxy clusters evaluated from X-ray images \|Yuan Z. S. Han J. L. \| MNRAS \| 513-3013 \| 2022 \| 2022MNRAS.513.3013Y \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.513.3013Y 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 \|Iliu0107 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 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 New 511 keV Line Data Provide Strongest sub-GeV Dark Matter Constraints \|De la Torre Luque Pedro Balaji Shyam \| ApJ \| 973-L6 \| 2024 \| 2024ApJ...973L...6D \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...973L...6D
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2017-04-17T05:07:51Z/2018-01-09T20:37:45Z
Version	21.51_20241115_1113
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
Last Update	2026-06-19
Keywords	"weak lensing measurements", "massive cluster", "forthcoming cosmological", "total exposure", "XMM", "distant massive cluster", "subaru hsc survey", "scaling relations", "systematic multi wavelength", "cosmological parameters", "hsc survey", "systematic xray", "icm temperatures", "icm thermal evolution", "gas profiles", "uniform sample"
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', 21.51_20241115_1113, European Space Agency, https://doi.org/10.5270/esa-6go7m3t
Rights	Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.