A dataset provided by the European Space Agency

Name: Scaling Relations of Distant, SZ-confirmed XXL Galaxy Clusters
Published: 2016-02-23T23:00:00Z

Proposal ID	074243
Title	Scaling Relations of Distant, SZ-confirmed XXL Galaxy Clusters
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742430101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742430201 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742430301 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0742430401
DOI	https://doi.org/10.5270/esa-2dfk7jf
Principal Investigator, PI	Dr Adam Mantz
Abstract	We propose to follow up four distant galaxy clusters discovered by the XMM-LSSand XXL survey programs. In addition to being confirmed with optical and NIRspectroscopy or photometry, the presence of hot gas in each of these clustershas been confirmed through a significant detection of the Sunyaev-Zel dovichsignal with CARMA. Three of our targets have redshifts greater than 1, with oneof them at 1.5. Deeper XMM data will allow us to situate these high-redshiftclusters on X-ray and SZ scaling relations and provide key mass proxies,enhancing the cosmological power of the XXL survey and enabling a variety ofstudies of cluster evolution. We also request joint Chandra observations inorder to constrain and remove point-source contamination of the XMM signal for these faint clusters.
Publications	The XXL Survey. XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters \|Koulouridis E. Poggianti B. et al. \| A&A \| 592-11 \| 2016 \| 2016A&A...592A..11K \| http://ui.adsabs.harvard.edu/#abs/2016A&A...592A..11K 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 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 composite X-ray spectra of radio-loud and radio-quiet SDSS quasars \|Zhou Min-Hua Gu Min-Feng \| RAA \| 21-4 \| 2021 \| 2021RAA....21....4Z \| http://ui.adsabs.harvard.edu/#abs/2021RAA....21....4Z 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 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 Probing the Origin of Changing-look Quasar Transitions with Chandra \|Yang Qian Green Paul J. et al. \| ApJ \| 953-61 \| 2023 \| 2023ApJ...953...61Y \| http://ui.adsabs.harvard.edu/#abs/2023ApJ...953...61Y 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 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 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 X-ray spectral properties of dust-obscured galaxies in the XMM-SERVS coverage of the XMM-LSS field \|Kayal Abhijit Singh Veeresh \| MNRAS \| 531-830 \| 2024 \| 2024MNRAS.531..830K \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.531..830K 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	2014-06-29T04:28:48Z/2015-02-07T23:11:38Z
Version	PPS_NOT_AVAILABLE
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	2016-02-23T23:00:00Z
Last Update	2025-01-27
Keywords	"cosmological power", "xmm lss", "deeper xmm data", "xmm signal", "scaling relations", "distant galaxy cluster", "sz scaling relations", "xxl survey", "faint clusters", "key mass proxies", "redshift cluster", "XMM", "nir spectroscopy", "cluster evolution", "xxl galaxy clusters", "hot gas", "xxl survey programs", "source contamination"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Adam Mantz, 2016, 'Scaling Relations of Distant, SZ-confirmed XXL Galaxy Clusters', PPS_NOT_AVAILABLE, European Space Agency, https://doi.org/10.5270/esa-2dfk7jf