A dataset provided by the European Space Agency

Name: eeHIFLUGCS: X-Ray Masses for a Complete Sample of about 400 Galaxy Clusters
Published: 2017-04-08T22:00:00Z

Proposal ID	076502
Title	eeHIFLUGCS: X-Ray Masses for a Complete Sample of about 400 Galaxy Clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765020101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765020201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765020301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765020601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765020701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765020801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765021201
DOI	https://doi.org/10.5270/esa-43g3wlu
Principal Investigator, PI	Prof Thomas Reiprich
Abstract	Currently, the largest complete local X-ray cluster sample with full highquality X-ray coverage is HIFLUGCS. Its selection is based on the ROSAT All-SkySurvey and complete X-ray follow-up has been performed with Chandra andXMM-Newton, resulting in numerous applications in cluster physics and cosmology.The combination of high completeness, large sample size, and high qualityfollow-up has been crucial for this wide applicability. Here, we propose asixfold increase in sample size with a new complete high quality sample of virgul400clusters, eeHIFLUGCS. We demonstrate that this sample constitutes the ultimatestep before eROSITA and that this significantly increased statistics will enablesubstantial (factor virgul3) improvements in precision as well as qualitatively new tests.
Publications	The non-uniformity of galaxy cluster metallicity profiles \|Lovisari, L., Reiprich, T. H., \| MNRAS \| 483-540 \| 2019 \| 2019MNRAS.483..540L \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.483..540L Probing cosmic isotropy with a new X-ray galaxy cluster sample through the LX-T scaling relation \|Migkas, K., Schellenberger, G., et al. \| A&A \| 636-15 \| 2020 \| 2020A&A...636A..15M \| http://ui.adsabs.harvard.edu/#abs/2020A&A...636A..15M A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies \|Ojha, Vineet, Chand, Hum, et al. \| ApJ \| 896-95 \| 2020 \| 2020ApJ...896...95O \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...896...95O 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 Cosmological implications of the anisotropy of ten galaxy cluster scaling relations \|Migkas, K., Pacaud, F., et al. \| A&A \| 649-151 \| 2021 \| 2021A&A...649A.151M \| http://ui.adsabs.harvard.edu/#abs/2021A&A...649A.151M 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	2015-06-03T23:57:13Z/2016-03-18T08:27:20Z
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	2017-04-08T22:00:00Z
Keywords	"quality sample", "sample constitutes", "complete xray", "wide applicability", "XMM", "quality xray coverage", "sample size", "numerous applications", "substantial factor", "cluster physics", "galaxy clusters", "increased statistics", "XMM-Newton", "xray masses", "complete sample", "ROSAT", "xmm newton", "sky survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Prof Thomas Reiprich, 2017, 'eeHIFLUGCS: X-Ray Masses for a Complete Sample of about 400 Galaxy Clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-43g3wlu