[en] The XXL survey currently covers two 25 sq. deg. patches with XMM observations of ~10ks. We summarise the scientific results associated with the first release of the XXL data set, that occurred mid 2016. We review several arguments for increasing the survey depth to 40 ks during the next decade of XMM operations. X-ray (z<2) cluster, (z<4) AGN and cosmic background survey science will then benefit from an extraordinary data reservoir. This, combined with deep multi-$\lambda$ observations, will lead to solid standalone cosmological constraints and provide a wealth of information on the formation and evolution of AGN, clusters and the X-ray background. In particular, it will offer a unique opportunity to pinpoint the z>1 cluster density. It will eventually constitute a reference study and an ideal calibration field for the upcoming eROSITA and Euclid missions.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Pierre, M.; Service d’Astrophysique du CEA, Saclay, FR
Surdej, Jean ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO)
The articles from the first XXL series quoted in the present paper are indicated with roman numbers in the reference list
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Eckert, D., et al. (2016). A&A, 592, A2 (XXL paper XIII).
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Koulouridis et al. (in preparation).
Le Brun A., et al. (2016). arXiv: 1606.04545.
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More information can be found on the website of: Hot Spots in the XMM Sky: Cosmology from X-ray to radio a prospective conference held in Mykonos (June 2016): http://www.astro.auth.gr/∼xmmcosmo16