A dataset provided by the European Space Agency

Name: eeHIFLUGCS: X-Ray Masses for a Complete Sample of about 400 Galaxy Clusters
Published: 2017-05-11T22:00:00Z

Proposal ID	076500
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=0765000101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765000301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765000401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765000601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765000701 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765000801 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765000901 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765001101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0765001201
DOI	https://doi.org/10.5270/esa-2tk5sch
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 A pre-merger stage galaxy cluster: Abell 3733 \|Kaya, H. Ilker, Caglar, Turgay, \| MNRAS \| 485-4550 \| 2019 \| 2019MNRAS.485.4550K \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.485.4550K 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 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 Low-frequency integrated radio spectra of diffuse, steep-spectrum sources in galaxy clusters: palaeontology with the MWA and ASKAP \|Duchesne, S. W., Johnston-Hollitt, M., \| PASA \| 38-53 \| 2021 \| 2021PASA...38...53D \| http://ui.adsabs.harvard.edu/#abs/2021PASA...38...53D 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	2015-06-23T08:41:41Z/2016-04-11T16:15:15Z
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	2017-05-11T22:00:00Z
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-2tk5sch