A dataset provided by the European Space Agency

Name: The ultimate XMM extragalactic survey SQUARE_BRACKET_OPENaSQUARE_BRACKET_CLOSE
Published: 2015-06-06T22:00:00Z

Proposal ID	074759
Title	The ultimate XMM extragalactic survey a
Download Data Associated to the proposal	https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590101 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590131 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590132 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590133 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590134 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590135 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590136 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590137 https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0747590801
DOI	https://doi.org/10.5270/esa-hve3phr
Principal Investigator, PI	Dr Marguerite Pierre
Abstract	We propose a 10-40ks/field XMM survey over 50 deg2, designed to constrain thedark energy equation of state using the 600 - 1,400 clusters of galaxies that wewill detect. The constraints that we will achieve on w_0 and w_a, of 0.7 and 2.4(10ks coverage) and 0.4 and 1.2 (40ks coverage) are at the level of the ultimateStage-IV DETF accuracy estimates achievable by cluster studies. This survey willalso have lasting legacy value for cluster scaling laws and studies of AGN andXRB.
Publications	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 X-ray constraints on the fraction of obscured active galactic nuclei at high accretion luminosities \|Georgakakis, A., Salvato, M., et al. \| MNRAS \| 469-3232 \| 2017 \| 2017MNRAS.469.3232G \| http://ui.adsabs.harvard.edu/#abs/2017MNRAS.469.3232G Estimating photometric redshifts for X-ray sources in the X-ATLAS field using machine-learning techniques \|Mountrichas, G., Corral, A., et al. \| A&A \| 608-39 \| 2017 \| 2017A&A...608A..39M \| http://ui.adsabs.harvard.edu/#abs/2017A&A...608A..39M Probing AGN inner structure with X-ray obscured type 1 AGN \|Liu, Teng, Merloni, Andrea, et al. \| MNRAS \| 479-5022 \| 2018 \| 2018MNRAS.479.5022L \| http://ui.adsabs.harvard.edu/#abs/2018MNRAS.479.5022L The XXL Survey. XXI. The environment and clustering of X-ray AGN in the XXL-South field \|Melnyk, O., Elyiv, A., et al. \| A&A \| 620-6 \| 2018 \| 2018A&A...620A...6M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...6M The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters \|Guglielmo, V., Poggianti, B. M., et al. \| A&A \| 620-7 \| 2018 \| 2018A&A...620A...7G \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...7G The XXL Survey. XIX. A realistic population of simulated X-ray AGN: Comparison of models with observations \|Koulouridis, E., Faccioli, L., et al. \| A&A \| 620-4 \| 2018 \| 2018A&A...620A...4K \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...4K The XXL Survey. XXIV. The final detection pipeline \|Faccioli, L., Pacaud, F., et al. \| A&A \| 620-9 \| 2018 \| 2018A&A...620A...9F \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...9F The XXL Survey: XXXIII. Chandra Constraints on the AGN Contamination of z > 1 XXL Galaxy Clusters \|Logan, C. H. A., Maughan, B. J., et al. \| A&A \| 620-18 \| 2018 \| 2018A&A...620A..18L \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A..18L The XXL Survey. XVI. The clustering of X-ray selected galaxy clusters at z 0.3 \|Marulli, F., Veropalumbo, A., et al. \| A&A \| 620-1 \| 2018 \| 2018A&A...620A...1M \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...1M The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy \|Farahi, Arya, Guglielmo, Valentina, et al. \| A&A \| 620-8 \| 2018 \| 2018A&A...620A...8F \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A...8F The XXL Survey: XXXIV. Double irony in XXL-North. A tale of two radio galaxies in a supercluster at z = 0.14 \|Horellou, C., Intema, H. T., et al. \| A&A \| 620-19 \| 2018 \| 2018A&A...620A..19H \| http://ui.adsabs.harvard.edu/#abs/2018A&A...620A..19H Mass--Richness Relations for X-Ray and SZE-selected Clusters at 0.4 < z < 2.0 as Seen by Spitzer at 4.5 mum \|Rettura, A., Chary, R., et al. \| ApJ \| 867-12 \| 2018 \| 2018ApJ...867...12R \| http://ui.adsabs.harvard.edu/#abs/2018ApJ...867...12R The Accretion History of AGNs. I. Supermassive Black Hole Population Synthesis Model \|Ananna, Tonima Tasnim, Treister, Ezequiel, et al. \| ApJ \| 871-240 \| 2019 \| 2019ApJ...871..240A \| http://ui.adsabs.harvard.edu/#abs/2019ApJ...871..240A Exploring the halo occupation of AGN using dark-matter cosmological simulations \|Georgakakis, A., Comparat, J., et al. \| MNRAS \| 487-275 \| 2019 \| 2019MNRAS.487..275G \| http://ui.adsabs.harvard.edu/#abs/2019MNRAS.487..275G Weak-lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data \|Umetsu, Keiichi, Sereno, Mauro, et al. \| ApJ \| 890-148 \| 2020 \| 2020ApJ...890..148U \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...890..148U The Clustering of X-Ray Luminous Quasars \|Powell, M. C., Urry, C. M., et al. \| ApJ \| 891-41 \| 2020 \| 2020ApJ...891...41P \| http://ui.adsabs.harvard.edu/#abs/2020ApJ...891...41P Candidate fossil groups in the CFHTLS: a probabilistic approach \|Adami, C., Sarron, F., et al. \| A&A \| 639-97 \| 2020 \| 2020A&A...639A..97A \| http://ui.adsabs.harvard.edu/#abs/2020A&A...639A..97A 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 HSC-XXL: Baryon budget of the 136 XXL groups and clusters \|Akino, Daichi, Eckert, Dominique, et al. \| PASJ \| 74-175 \| 2022 \| 2022PASJ...74..175A \| http://ui.adsabs.harvard.edu/#abs/2022PASJ...74..175A The XXL Survey. XLV. Linking the ages of optically selected groups to their X-ray emission \|Crossett, J. P., McGee, S. L., et al. \| A&A \| 663-2 \| 2022 \| 2022A&A...663A...2C \| http://ui.adsabs.harvard.edu/#abs/2022A&A...663A...2C The XXL survey. XLVI. Forward cosmological analysis of the C1 cluster sample \|Garrel, Christian, Pierre, Marguerite, et al. \| A&A \| 663-3 \| 2022 \| 2022A&A...663A...3G \| http://ui.adsabs.harvard.edu/#abs/2022A&A...663A...3G The co-evolution of supermassive black holes and galaxies in luminous AGN over a wide range of redshift \|Mountrichas, George, \| A&A \| 672-98 \| 2023 \| 2023A&A...672A..98M \| http://ui.adsabs.harvard.edu/#abs/2023A&A...672A..98M Association of optical, ultraviolet, and soft X-ray excess emissions in AGNs \|Nour, D., Sriram, K., \| MNRAS \| 518-5705 \| 2023 \| 2023MNRAS.518.5705N \| http://ui.adsabs.harvard.edu/#abs/2023MNRAS.518.5705N The XXL Survey. L. Active galactic nucleus contamination in galaxy clusters: Detection and cosmological impact \|Bhargava, Sunayana, Garrel, Christian, et al. \| A&A \| 673-92 \| 2023 \| 2023A&A...673A..92B \| http://ui.adsabs.harvard.edu/#abs/2023A&A...673A..92B Large-scale clustering of buried X-ray AGN: Trends in AGN obscuration and redshift evolution \|Viitanen, A., Allevato, V., et al. \| A&A \| 674-214 \| 2023 \| 2023A&A...674A.214V \| http://ui.adsabs.harvard.edu/#abs/2023A&A...674A.214V Link between star formation and the properties of supermassive black holes \|Mountrichas, George, Buat, V\\u00e9ronique, \| A&A \| 679-151 \| 2023 \| 2023A&A...679A.151M \| http://ui.adsabs.harvard.edu/#abs/2023A&A...679A.151M The intrinsic X-ray luminosity distribution of an optically selected SDSS quasar population \|Rankine, Amy L., Aird, James, et al. \| MNRAS \| 527-9004 \| 2024 \| 2024MNRAS.527.9004R \| http://ui.adsabs.harvard.edu/#abs/2024MNRAS.527.9004R 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 The Massive and Distant Clusters of WISE Survey 2: Equatorial First Data Release \|Thongkham, Khunanon, Gonzalez, Anthony H., et al. \| ApJ \| 967-123 \| 2024 \| 2024ApJ...967..123T \| http://ui.adsabs.harvard.edu/#abs/2024ApJ...967..123T Observed abundance of X-ray low surface brightness clusters in optical, X-ray, and SZ selected samples \|Andreon, S., Trinchieri, G., \| A&A \| 686-A284 \| 2024 \| 2024A&A...686A.284A \| http://ui.adsabs.harvard.edu/#abs/2024A&A...686A.284A 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	2014-05-11T01:38:15Z/2014-05-12T10:37:31Z
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	2015-06-06T22:00:00Z
Keywords	"dark energy equation", "XMM", "cluster scaling laws", "xmm extragalactic survey", "field xmm survey"
Publisher And Registrant	European Space Agency
Credit Guidelines	European Space Agency, Dr Marguerite Pierre, 2015, 'The ultimate XMM extragalactic survey SQUARE_BRACKET_OPENaSQUARE_BRACKET_CLOSE', 17.56_20190403_1200, European Space Agency, https://doi.org/10.5270/esa-hve3phr