A dataset provided by the European Space Agency

Name: A systematic study of z>1 XXL galaxy clusters
Published: 2020-02-19T23:00:00Z

Proposal ID	082125
Title	A systematic study of z>1 XXL galaxy clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821250401 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821250501 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821250601 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0821250701
DOI	https://doi.org/10.5270/esa-y8qqwg2
Principal Investigator, PI	Dr Ben Maughan
Abstract	The XXL survey has constructed the most pure and reliable sample of distant(z>1) X-ray-selected clusters of galaxies, thanks to its well-calibratedselection function and our complete Chandra follow-up to identify anycontaminating point sources. In this proposal we initiate a programme of deeperXMM observations of these clusters to measure their properties and evolution,examine their morphologies, compare them with distant SZE-selected clusters, andprobe the parameter space where distant eROSITA clusters will be found. Werequest 268 ks to observe three clusters, completing an initial sample of sixChandra-validated z>1 XXL clusters.
Publications	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 XXL Survey - XLVIII. X-ray follow-up of distant XXL clusters: masses scaling relations and AGN contamination \|Duffy R. T. Logan C. H. A. et al. \| MNRAS \| 512-2525 \| 2022 \| 2022MNRAS.512.2525D \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.512.2525D 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
Instrument	EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage	2018-05-13T03:06:36Z/2019-02-06T03:37:02Z
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	2020-02-19T23:00:00Z
Last Update	2025-01-27
Keywords	"parameter space", "xxl clusters", "complete chandra", "initial sample", "xxl survey", "deeper xmm", "chandra validated z", "distant z", "distant sze", "XMM", "distant erosita cluster", "xxl galaxy clusters", "reliable sample", "calibrated selection function"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Ben Maughan, 2020, 'A systematic study of z>1 XXL galaxy clusters', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-y8qqwg2