A dataset provided by the European Space Agency

Name: Deep Observation of an SZ-confirmed XXL Galaxy Cluster at Redshift 1.9
Published: 2016-07-29T22:00:00Z

Proposal ID	076054
Title	Deep Observation of an SZ-confirmed XXL Galaxy Cluster at Redshift 1.9
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0760540101
DOI	https://doi.org/10.5270/esa-ju5lvjy
Principal Investigator, PI	Dr Adam Mantz
Abstract	We propose a deep 100 ks observation of XLSSU J021744.1-034536, a galaxy clusterdiscovered by the XMM-LSS survey. The cluster was confirmed through optical andNIR imaging, and has 10-band photometric data indicating the very high redshiftof z=1.9. We obtained a high-significance detection of the Sunyaev-Zeldovicheffect of this system, confirming the presence of hot gas and providing anestimate of the cluster mass (1-2 10^14 Msun). The proposed observations willallow us to measure key properties of the intracluster medium, namely the gasmass, temperature and center-excised luminosity. The data will provide an anchorfor extending our understanding of cluster growth and scaling relations to highredshifts, and will enhance the cosmological power of the XMM-XXL survey.
Publications	The XMM-SERVS survey: new XMM-Newton point-source catalogue for the XMM-LSS field \|Chen C.-T. J. Brandt W. N. et al. \| MNRAS \| 478-2132 \| 2018 \| 2018MNRAS.478.2132C \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.478.2132C The XXL Survey. XVII. X-ray and Sunyaev-Zeldovich properties of the redshift 2.0 galaxy cluster XLSSC 122 \|Mantz A. B. Abdulla Z. et al. \| A&A \| 620-2 \| 2018 \| 2018A&A...620A...2M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...2M Spectroscopic confirmation of a mature galaxy cluster at a redshift of 2 \|Willis J. P. Canning R. E. A. et al. \| Natur \| 577-39 \| 2020 \| 2020Natur.577...39W \| http://ui.adsabs.harvard.edu/#abs/2020Natur.577...39W 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 Implications of the Environments of Radio-detected Active Galactic Nuclei in a Complex Protostructure at z u223c 3.3 \|Shen Lu Lemaux Brian C. et al. \| ApJ \| 912-60 \| 2021 \| 2021ApJ...912...60S \| http://ui.adsabs.harvard.edu/#abs/2021ApJ...912...60S 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 Consistent Analysis of the AGN LF in X-Ray and MIR in the XMM-LSS Field \|Runburg Jack Farrah Duncan et al. \| ApJ \| 924-133 \| 2022 \| 2022ApJ...924..133R \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...924..133R 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 A fresh look at AGN spectral energy distribution fitting with the XMM-SERVS AGN sample \|Marshall Adam Auger-Williams Matthew W. et al. \| MNRAS \| 515-5617 \| 2022 \| 2022MNRAS.515.5617M \| http://ui.adsabs.harvard.edu/#abs/2022MNRAS.515.5617M The Obscured Fraction of Quasars at Cosmic Noon \|Vijarnwannaluk Bovornpratch Akiyama Masayuki et al. \| ApJ \| 941-97 \| 2022 \| 2022ApJ...941...97V \| http://ui.adsabs.harvard.edu/#abs/2022ApJ...941...97V Detection of radio-AGN in dust-obscured galaxies using deep uGMRT radio continuum observations \|Kayal Abhijit Singh Veeresh et al. \| JApA \| 43-84 \| 2022 \| 2022JApA...43...84K \| http://ui.adsabs.harvard.edu/#abs/2022JApA...43...84K Search and Characterization of Remnant Radio Galaxies in the XMM-LSS Deep Field \|Dutta Sushant Singh Veeresh et al. \| ApJ \| 944-176 \| 2023 \| 2023ApJ...944..176D \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...944..176D The Most Obscured AGNs in the XMM-SERVS Fields \|Yan Wei Brandt W. N. et al. \| ApJ \| 951-27 \| 2023 \| 2023ApJ...951...27Y \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...951...27Y The LSST AGN Data Challenge: Selection Methods \|Saviu0107 u0110oru0111e V. Jankov Isidora et al. \| ApJ \| 953-138 \| 2023 \| 2023ApJ...953..138S \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...953..138S Observational properties of active galactic nucleus obscuration during the peak of accretion growth \|Vijarnwannaluk Bovornpratch Akiyama Masayuki et al. \| MNRAS \| 529-3610 \| 2024 \| 2024MNRAS.529.3610V \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.529.3610V 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	2015-07-16T06:30:06Z/2015-07-17T12:06:46Z
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	2016-07-29T22:00:00Z
Last Update	2025-01-27
Keywords	"cosmological power", "cluster growth", "key properties", "scaling relations", "center excised luminosity", "xmm lss survey", "cluster mass", "intracluster medium", "xmm xxl survey", "nir imaging", "sunyaev zeldovich effect", "xxl galaxy cluster", "galaxy cluster", "significance detection", "XMM", "gas mass", "hot gas", "xlssu j021744", "band photometric data"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Adam Mantz, 2016, 'Deep Observation of an SZ-confirmed XXL Galaxy Cluster at Redshift 1.9', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-ju5lvjy