A dataset provided by the European Space Agency

Name: Complete High Precision Study of Galaxy Clusters for Modern Cosmology
Published: 2015-01-20T23:00:00Z

Proposal ID	072189
Title	Complete High Precision Study of Galaxy Clusters for Modern Cosmology
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721890101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721890201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721890401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0721890501
DOI	https://doi.org/10.5270/esa-2cu6ydi
Principal Investigator, PI	Dr Yu-Ying Zhang
Abstract	We request 109~ks data for 4 clusters to complete a volume-limited sample of 51clusters at 0.15
Publications	XMM-Newton publication statistics \|Ness J.-U. Parmar A. N. et al. \| AN \| 335-210 \| 2014 \| 2014AN....335..210N \| http://ui.adsabs.harvard.edu/#abs/2014AN....335..210N The Million Optical - Radio/X-ray Associations (MORX) Catalogue \|Flesch Eric W. \| PASA \| 33-52 \| 2016 \| 2016PASA...33...52F \| http://ui.adsabs.harvard.edu/#abs/2016PASA...33...52F Searching for gamma-ray signature in WHSP blazars. Fermi-LAT detection of 150 excess signal in the 0.3-500 GeV band \|Arsioli B. Chang Y.-L. \| A&A \| 598-134 \| 2017 \| 2017A&A...598A.134A \| http://ui.adsabs.harvard.edu/#abs/2017A&A...598A.134A The XMM Cluster Survey: new evidence for the 3.5-keV feature in clusters is inconsistent with a dark matter origin \|Bhargava S. Giles P. A. et al. \| MNRAS \| 497-656 \| 2020 \| 2020MNRAS.497..656B \| http://ui.adsabs.harvard.edu/#abs/2020MNRAS.497..656B 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 Imaging results from the legacy Giant Metrewave Radio Telescope Galaxy Cluster Key Project \|George Lijo T. Kale Ruta \| MNRAS \| 507-4487 \| 2021 \| 2021MNRAS.507.4487G \| http://ui.adsabs.harvard.edu/#abs/2021MNRAS.507.4487G 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	2013-07-17T02:49:13Z/2013-12-30T21:52:10Z
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	2015-01-20T23:00:00Z
Last Update	2025-01-27
Keywords	"modern cosmology", "sz effect", "inadvertent selection biases", "future surveys", " yx", "cluster cosmology surveys", "noted mass", "low scatter", "galaxy cluster", "fit scaling relations", "xray mass proxies", ".", "systematic biases", "mass bias", "volume limited sample", "deliver definitive constraints", "main limitation"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Yu-Ying Zhang, 2015, 'Complete High Precision Study of Galaxy Clusters for Modern Cosmology', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-2cu6ydi