A dataset provided by the European Space Agency

Name 065534
Title XMM guided survey of the CFHTLS: a Milestone for X-ray Cluster Cosmology
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340131
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340132
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340133
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340134
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340135
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340136
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340137
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340138
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340139
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340140
...
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340141
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340142
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340143
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340144
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340145
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340146
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340147
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340148
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340149
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340150
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340151
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340152
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340153
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340154
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340155
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340156
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340157
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340158
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340159
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340160
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655340161
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343831
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343832
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343833
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343834
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343835
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343836
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343837
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343838
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343839
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343840
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343841
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343842
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343843
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343844
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343845
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343846
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343847
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343848
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343849
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343850
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343851
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343852
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343853
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343854
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343855
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343856
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343857
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343858
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343859
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343860
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655343861
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346801
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346831
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346832
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346833
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346834
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346835
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346836
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346837
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346838
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346839
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346840
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346841
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346842
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655346843
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0655348101

DOI 10.5270/esa-rhrmabu
Author Dr ALEXIS FINOGUENOV
Description Both X-rays and gravitational lensing are highly recognized paths to carry out cosmological studies, with several space missions being prepared: eROSITA, EUCLIDE, JDEM. Galaxy clusters which are going to be found in all those surveys will provide a quantum leap in our understanding of the Cosmology. We propose here a unique path-finder survey optimized for a joint X-ray and gravitational lensing cluster detection in the redshift range of 0.1-1. This proposal is a joint program on calibrating and extending the 400 square degree survey to pursue the measurement of dark energy to 3% accuracy achieved in a combination with WMAP, BAO and SN experiments.
Publication XMM-Newton publication statistics . Ness, J.-U., Parmar, A. N., et all. . AN . 335-210 . 2014 . 2014AN....335..210N ,
Statistical properties of dwarf novae-type cataclysmic variables: the outburst catalogue . Coppejans, Deanne L., Kording, Elmar G., et all. . MNRAS . 456-4441 . 2016 . 2016MNRAS.456.4441C ,
The XXL Survey. XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters . Koulouridis, E., Poggianti, B., et all. . A&A . 592-11 . 2016 . 2016A&A...592A..11K ,
Spectral clustering for optical confirmation and redshift estimation of X-ray selected galaxy cluster candidates in the SDSS Stripe 82 . Mahmoud, E., Takey, A., . A&C . 16-174 . 2016 . 2016A&C....16..174M ,
Ensemble X-ray variability of active galactic nuclei. II. Excess variance and updated structure function . Vagnetti, F., Middei, R., et all. . A&A . 593-55 . 2016 . 2016A&A...593A..55V ,
The 3XMM-SDSS Stripe 82 Galaxy Cluster Survey. I. Cluster catalogue and discovery of two merging cluster candidates . Takey, A., Durret, F., et all. . A&A . 594-32 . 2016 . 2016A&A...594A..32T ,
The Million Optical - Radio-X-ray Associations (MORX) Catalogue . Flesch, Eric W., . PASA . 33-52 . 2016 . 2016PASA...33...52F ,
A new sample of X-ray selected narrow emission-line galaxies. II. Looking for True Seyfert 2 . Pons, E., Watson, M. G., . A&A . 594-72 . 2016 . ...,
Dependence of the broad Fe Kalpha line on the physical parameters of AGN . Liu, Zhu, Yuan, Weimin, et all. . MNRAS . 463-684 . 2016 . 2016MNRAS.463..684L ,
M Dwarf Activity in the Pan-STARRS1 Medium-Deep Survey: First Catalog and Rotation Periods . Kado-Fong, E., Williams, P. K. G., et all. . ApJ . 833-281 . 2016 . 2016ApJ...833..281K ,
Searching for gamma-ray signature in WHSP blazars. Fermi-LAT detection of 150 excess signal in the 0.3-500 GeV band . Arsioli, B., Chang, Y.-L., . A&A . 598-134 . 2017 . 2017A&A...598A.134A ,
Multiwavelength study of X-ray luminous clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field . Miyaoka, Keita, Okabe, Nobuhiro, et all. . PASJ . 70-22 . 2018 . 2018PASJ...70S..22M ,
Constraining the Dark-matter Halo Mass of Isolated Low-surface-brightness Galaxies . Kovacs, Orsolya E., Bogdan, Akos, . ApJ . 879-12 . 2019 . 2019ApJ...879L..12K ,
The 3XMM-SDSS Stripe 82 Galaxy Cluster Survey - II. X-ray and optical properties of the cluster sample . Takey, Ali, Durret, Florence, et all. . MNRAS . 486-4863 . 2019 . 2019MNRAS.486.4863T ,
X-ray properties of high-richness CAMIRA clusters in the Hyper Suprime-Cam Subaru Strategic Program field . Ota, Naomi, Mitsuishi, Ikuyuki, et all. . PASJ . 72-1 . 2020 . 2020PASJ...72....1O ,
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 ,
The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters . Pastor-Marazuela, I., Webb, N. A., et all. . A&A . 640-124 . 2020 . 2020A&A...640A.124P ,
A new multiwavelength census of blazars . Paggi, A., Bonato, M., et all. . A&A . 641-62 . 2020 . 2020A&A...641A..62P ,
Instrument EPN, OM, RGS1, RGS2, EMOS1, EMOS2
Temporal Coverage 2010-10-22T22:50:32Z/2011-01-22T03:18:30Z
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 2012-02-08T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-02-08T00:00:00Z, 065534, 17.56_20190403_1200. https://doi.org/10.5270/esa-rhrmabu