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The XXL survey: First results and future

dc.contributor.authorPierre, M.
dc.contributor.authorAdami, C.
dc.contributor.authorBirkinshaw, M.
dc.contributor.authorChiappetti, L.
dc.contributor.authorEttori, S.
dc.contributor.authorEvrard, A.
dc.contributor.authorFaccioli, L.
dc.contributor.authorGastaldello, F.
dc.contributor.authorGiles, P.
dc.contributor.authorHorellou, C.
dc.contributor.authorIovino, A.
dc.contributor.authorKoulouridis, E.
dc.contributor.authorLidman, C.
dc.contributor.authorLe Brun, A.
dc.contributor.authorMaughan, B.
dc.contributor.authorMaurogordato, S.
dc.contributor.authorMcCarthy, I.
dc.contributor.authorMiyazaki, S.
dc.contributor.authorPacaud, F.
dc.contributor.authorPaltani, S.
dc.contributor.authorPlionis, M.
dc.contributor.authorReiprich, T.
dc.contributor.authorSadibekova, T.
dc.contributor.authorSmolcic, V.
dc.contributor.authorSnowden, S.
dc.contributor.authorSurdej, J.
dc.contributor.authorTsirou, M.
dc.contributor.authorVignali, C.
dc.contributor.authorWillis, J.
dc.contributor.authorAlis, S.
dc.contributor.authorAltieri, B.
dc.contributor.authorBaran, N.
dc.contributor.authorBenoist, C.
dc.contributor.authorBongiorno, A.
dc.contributor.authorBremer, M.
dc.contributor.authorButler, A.
dc.contributor.authorCappi, A.
dc.contributor.authorCaretta, C.
dc.contributor.authorCiliegi, P.
dc.contributor.authorClerc, N.
dc.contributor.authorCorasaniti, P.
dc.contributor.authorCoupon, J.
dc.contributor.authorDelhaize, J.
dc.contributor.authorDelvecchio, I.
dc.contributor.authorDemocles, J.
dc.contributor.authorDesai, S.
dc.contributor.authorDevriendt, J.
dc.contributor.authorDubois, Y.
dc.contributor.authorEckert, D.
dc.contributor.authorElyiv, A.
dc.contributor.authorFarahi, A.
dc.contributor.authorFerraril, C.
dc.contributor.authorFotopoulou, S.
dc.contributor.authorForman, W.
dc.contributor.authorGeorgantopoulos, I.
dc.contributor.authorGuglielmo, V.
dc.contributor.authorHuynh, M.
dc.contributor.authorJerlin, N.
dc.contributor.authorJones, C.
dc.contributor.authorLavoie, S.
dc.contributor.authorLe Fevre, J.
dc.contributor.authorLieu, M.
dc.contributor.authorKilbinger, M.
dc.contributor.authorMaruIli, F.
dc.contributor.authorMantz, A.
dc.contributor.authorMcGee, S.
dc.contributor.authorMelin, J.
dc.contributor.authorMelnyk, O.
dc.contributor.authorMoscardini, L.
dc.contributor.authorNovak, M.
dc.contributor.authorPiconcelli, E.
dc.contributor.authorPoggianti, B.
dc.contributor.authorPomarede, D.
dc.contributor.authorPompei, E.
dc.contributor.authorPonman, T.
dc.contributor.authorRamos Ceja, M.
dc.contributor.authorRana, P.
dc.contributor.authorRapetti, D.
dc.contributor.authorRaychaudhury, S.
dc.contributor.authorRicci, M.
dc.contributor.authorRottgering, H.
dc.contributor.authorSahlen, M.
dc.contributor.authorSauvageot, J.
dc.contributor.authorSchimd, C.
dc.contributor.authorSereno, M.
dc.contributor.authorSmith, G.
dc.contributor.authorUmetsu, K.
dc.contributor.authorValageas, P.
dc.contributor.authorValotti, A.
dc.contributor.authorValtchanov, I.
dc.contributor.authorVeropalumbo, A.
dc.contributor.authorAscaso, B.
dc.contributor.authorBarnes, D.
dc.contributor.authorDe Petris, M.
dc.contributor.authorDurret, F.
dc.contributor.authorDonahue, M.
dc.contributor.authorIthana, M.
dc.contributor.authorJarvis, M.
dc.contributor.authorJohnston-Hollitt, Melanie
dc.date.accessioned2018-12-13T09:15:19Z
dc.date.available2018-12-13T09:15:19Z
dc.date.created2018-12-12T02:46:57Z
dc.date.issued2017
dc.identifier.citationPierre, M. and Adami, C. and Birkinshaw, M. and Chiappetti, L. and Ettori, S. and Evrard, A. and Faccioli, L. et al. 2017. The XXL survey: First results and future. Astronomische Nachrichten. 338 (2-3): pp. 334-341.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/73060
dc.identifier.doi10.1002/asna.201713352
dc.description.abstract

© 2017 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim The XXL survey currently covers two 25 deg2patches with XMM observations of ~10 ks. We summarize the scientific results associated with the first release of the XXL dataset, which occurred in 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) active galactic nuclei (AGN), and cosmic background survey science will then benefit from an extraordinary data reservoir. This, combined with deep multi-? 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.
dc.publisherWiley - V C H Verlag GmbH & Co. KGaA
dc.titleThe XXL survey: First results and future
dc.typeJournal Article
dcterms.source.volume338
dcterms.source.number2-3
dcterms.source.startPage334
dcterms.source.endPage341
dcterms.source.issn0004-6337
dcterms.source.titleAstronomische Nachrichten
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusFulltext not available


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