A dataset provided by the European Space Agency

Name 074719
Title The ultimate XMM extragalactic survey [a]
URL

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DOI 10.5270/esa-dj8q986
Author Dr Marguerite Pierre
Description We propose a 10-40ks-field XMM survey over 50 deg2, designed to constrain the dark energy equation of state using the 600 - 1,400 clusters of galaxies that we will 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 ultimate Stage-IV DETF accuracy estimates achievable by cluster studies. This survey will also have lasting legacy value for cluster scaling laws and studies of AGN and XRB.
Publication The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
X-ray constraints on the fraction of obscured active galactic nuclei at high accretion luminosities . Georgakakis, A., Salvato, M., et all. . MNRAS . 469-3232 . 2017 . 2017MNRAS.469.3232G ,
Estimating photometric redshifts for X-ray sources in the X-ATLAS field using machine-learning techniques . Mountrichas, G., Corral, A., et all. . A&A . 608-39 . 2017 . 2017A&A...608A..39M ,
Probing AGN inner structure with X-ray obscured type 1 AGN . Liu, Teng, Merloni, Andrea, et all. . MNRAS . 479-5022 . 2018 . 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 all. . A&A . 620-6 . 2018 . 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 all. . A&A . 620-7 . 2018 . 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 all. . A&A . 620-4 . 2018 . 2018A&A...620A...4K ,
The XXL Survey. XXIV. The final detection pipeline . Faccioli, L., Pacaud, F., et all. . A&A . 620-9 . 2018 . ...,
The XXL Survey: XXXIII. Chandra Constraints on the AGN Contamination of z > 1 XXL Galaxy Clusters . Logan, C. H. A., Maughan, B. J., et all. . A&A . 620-18 . 2018 . 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 all. . A&A . 620-1 . 2018 . 2018A&A...620A...1M ,
The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy . Farahi, Arya, Guglielmo, Valentina, et all. . A&A . 620-8 . 2018 . 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 all. . A&A . 620-19 . 2018 . 2018A&A...620A..19H ,
Mass--Richness Relations for X-Ray and SZE-selected Clusters at 0.4xa0 2018ApJ...867...12R ,
The Accretion History of AGNs. I. Supermassive Black Hole Population Synthesis Model . Ananna, Tonima Tasnim, Treister, Ezequiel, et all. . ApJ . 871-240 . 2019 . 2019ApJ...871..240A ,
Exploring the halo occupation of AGN using dark-matter cosmological simulations . Georgakakis, A., Comparat, J., et all. . MNRAS . 487-275 . 2019 . 2019MNRAS.487..275G ,
Constraining the Dark-matter Halo Mass of Isolated Low-surface-brightness Galaxies . Kovacs, Orsolya E., Bogdan, Akos, . ApJ . 879-12 . 2019 . 2019ApJ...879L..12K ,
Weak-lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data . Umetsu, Keiichi, Sereno, Mauro, et all. . ApJ . 890-148 . 2020 . 2020ApJ...890..148U ,
The Clustering of X-Ray Luminous Quasars . Powell, M. C., Urry, C. M., et all. . ApJ . 891-41 . 2020 . 2020ApJ...891...41P ,
On the Relation between the Hard X-Ray Photon Index and Accretion Rate for Super-Eddington Accreting Quasars . Huang, Jian, Luo, Bin, et all. . ApJ . 895-114 . 2020 . 2020ApJ...895..114H ,
A Comparison of X-Ray Photon Indices among the Narrow- and Broad-line Seyfert 1 Galaxies . Ojha, Vineet, Chand, Hum, et all. . ApJ . 896-95 . 2020 . 2020ApJ...896...95O ,
Candidate fossil groups in the CFHTLS: a probabilistic approach . Adami, C., Sarron, F., et all. . A&A . 639-97 . 2020 . 2020A&A...639A..97A ,
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2014-01-30T11:29:50Z/2015-02-05T18:07:33Z
Version 17.56_20190403_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's 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 Earth's 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 2016-02-16T23:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2016-02-16T23:00:00Z, 074719, 17.56_20190403_1200. https://doi.org/10.5270/esa-dj8q986