A dataset provided by the European Space Agency

Name 067766
Title The ultimate XMM extragalactic survey [a]
URL

http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660101
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660201
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660231
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660232
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660233
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660234
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660235
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660236
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660237
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660238
http://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0677660239
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DOI 10.5270/esa-6d8urk8
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 Serendipitous UV source catalogues for 10 years of XMM and 5 years of Swift . Yershov, V. N., . Ap&SS . 354-97 . 2014 . 2014Ap&SS.354...97Y ,
The XXL Survey. I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme . Pierre, M., Pacaud, F., et all. . A&A . 592-1 . 2016 . 2016A&A...592A...1P ,
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 ,
The XXL Survey. II. The bright cluster sample: catalogue and luminosity function . Pacaud, F., Clerc, N., et all. . A&A . 592-2 . 2016 . 2016A&A...592A...2P ,
The XXL Survey. III. Luminosity-temperature relation of the bright cluster sample . Giles, P. A., Maughan, B. J., et all. . A&A . 592-3 . 2016 . 2016A&A...592A...3G ,
The XXL Survey . IV. Mass-temperature relation of the bright cluster sample . Lieu, M., Smith, G. P., et all. . A&A . 592-4 . 2016 . 2016A&A...592A...4L ,
The XXL Survey. VI. The 1000 brightest X-ray point sources . Fotopoulou, S., Pacaud, F., et all. . A&A . 592-5 . 2016 . 2016A&A...592A...5F ,
The XXL Survey. VII. A supercluster of galaxies at z = 0.43 . Pompei, E., Adami, C., et all. . A&A . 592-6 . 2016 . 2016A&A...592A...6P ,
The...
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2012-07-20T00:00:46Z/2012-07-21T14:22:41Z
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 2012-08-02T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2012-08-02T00:00:00Z, 067766, 17.56_20190403_1200. https://doi.org/10.5270/esa-6d8urk8