Reference : The XXL survey: First results and future
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/218220
The XXL survey: First results and future
English
Pierre, M. [Service d’Astrophysique du CEA, Saclay, FR > > > >]
Adami, C. [Laboratoire d’Astrophysique, Marseille, FR > > > >]
Birkinshaw, M. [University of Bristol, UK > > > >]
Chiappetti, L. [INAF-IASF, Milano, IT > > > >]
Ettori, S. [NAF-OABO, Bologna, IT > > > >]
Evrard, A. [University of Michigan, Ann Arbor, US > > > >]
Faccioli, L. [> >]
Gastaldello, F. [> >]
Giles, P. [> >]
Horellou, C. [> >]
Iovino, A. [> >]
Koulouridis, E. [> >]
Lidman, C. [> >]
Le Brun, A. []
Maughan, B. [> >]
Maurogordato, S. [> >]
McCarthy, I. [> >]
Miyazaki, S. [> >]
Pacaud, F. [> >]
Paltani, S. [> >]
Plionis, M. [> >]
Reiprich, T. [> >]
Sadibekova, T. [> >]
Smolcic, V. [> >]
Snowden, S. [> >]
Surdej, Jean mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Département d'astrophys., géophysique et océanographie (AGO) >]
Tsirou, M. [> >]
Vignali, C. [> >]
Willis, J. [> >]
Alis, S. [> >]
Altieri, B. [> >]
Baran, N. [> >]
Benoist, C. [> >]
Bongiorno, A. [> >]
Bremer, M. [> >]
Butler, A. [> >]
Cappi, A. [> >]
Caretta, C. [> >]
Ciliegi, P. [> >]
Clerc, N. [> >]
Corasaniti, P. S. [> >]
Coupon, J. [> >]
Delhaize, J. [> >]
Delvecchio, I. [> >]
Democles, J. [> >]
Desai, Sh [> >]
Devriendt, J. [> >]
Dubois, Y. []
Eckert, D. [> >]
Elyiv, A. [> >]
Farahi, A. [> >]
Ferraril, C. [> >]
Fotopoulou, S. [> >]
Forman, W. [> >]
Georgantopoulos, I. [> >]
Guglielmo, V. [> >]
Huynh, M. [> >]
Jerlin, N. [> >]
Jones, Ch [> >]
Lavoie, S. [> >]
Le Fevre, J.-P. [> >]
Lieu, M. [> >]
Kilbinger, M. [> >]
MaruIli, F. [> >]
Mantz, A. [> >]
McGee, S. [> >]
Melin, J.-B. [> >]
Melnyk, O. [> >]
Moscardini, L. [> >]
Novak, M. [> >]
Piconcelli, E. [> >]
Poggianti, B. [> >]
Pomarede, D. [> >]
Pompei, E. [> >]
Ponman, T. [> >]
Ramos Ceja, M. E. [> >]
Rana, P. [> >]
Rapetti, D. [> >]
Raychaudhury, S. [> >]
Ricci, M. [> >]
Rottgering, H. [> >]
Sahlen, M. [> >]
Sauvageot, J.-L. [> >]
Schimd, C. [> >]
Sereno, M. [> >]
Smith, G. P. [> >]
Umetsu, K. [> >]
Valageas, P. [> >]
Valotti, A. [> >]
Valtchanov, I. [> >]
Veropalumbo, A. [> >]
Ascaso, B. [> >]
Barnes, D. [> >]
De Petris, M. [> >]
Durret, F. [> >]
Donahue, M. [> >]
Ithana, M. [> >]
Jarvis, M. [> >]
Johnston-Hollitt, M. [> >]
Kalfountzou, E. [> >]
Kay, S. [> >]
La Franca, F. [> >]
Okabe, N. [> >]
Muzzin, A. [> >]
Rettura, A. [> >]
Ricci, F. []
Ridl, J. [> >]
Risaliti, G. [> >]
Takizawa, M. [> >]
Thomas, P. [> >]
Truong, N. [> >]
1-Mar-2017
Astronomische Nachrichten
Wiley
338
334-341
Yes (verified by ORBi)
International
0004-6337
1521-3994
Berlin
Germany
[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.
Researchers ; Professionals
http://hdl.handle.net/2268/218220
10.1002/asna.201713352
http://esoads.eso.org/abs/2017AN....338..334P

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