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dc.contributor.authorPonman, T. J.
dc.contributor.authorCHIAPPETTI, L.
dc.contributor.authorDemocles, J.
dc.contributor.authorECKERT, D.
dc.contributor.authorEVRARD, A. E.
dc.contributor.authorFACCIOLI, L.
dc.contributor.authorGASTALDELLO, F.
dc.contributor.authorGUENNOU, L.
dc.contributor.authorHorellou, C.
dc.contributor.authorTUFFS, R.
dc.contributor.authorPACAUD, F.
dc.contributor.authorCLERC, N.
dc.contributor.authorGiles, P. A.
dc.contributor.authorADAMI, C.
dc.contributor.authorSADIBEKOVA, T.
dc.contributor.authorPIERRE, M.
dc.contributor.authorMaughan, B. J.
dc.contributor.authorLieu, M.
dc.contributor.authorLE FEVRE, J. P.
dc.contributor.authorSmith, G. P.
dc.contributor.authorVALAGEAS, P.
dc.contributor.authorVALTCHANOV, I.
dc.contributor.authorWillis, J. P.
dc.contributor.authorZiparo, F.
dc.contributor.authorAlis, Sinan
dc.contributor.authorIOVINO, A.
dc.contributor.authorKOULOURIDIS, E.
dc.contributor.authorLE BRUN, V.
dc.contributor.authorLIDMAN, C.
dc.contributor.authorLiske, J.
dc.contributor.authorMAUROGORDATO, S.
dc.contributor.authorMENANTEAU, F.
dc.contributor.authorOWERS, M.
dc.contributor.authorPOGGIANTI, B.
dc.contributor.authorPOMAREDE, D.
dc.contributor.authorPOMPEI, E.
dc.contributor.authorRapetti, D.
dc.contributor.authorREIPRICH, T. H.
dc.contributor.authorALTIERI, B.
dc.contributor.authorARDILA, F.
dc.contributor.authorBaldry, I.
dc.contributor.authorBENOIST, C.
dc.contributor.authorBirkinshaw, M.
dc.date.accessioned2021-03-05T09:58:45Z
dc.date.available2021-03-05T09:58:45Z
dc.identifier.citationPACAUD F., CLERC N., Giles P. A. , ADAMI C., SADIBEKOVA T., PIERRE M., Maughan B. J. , Lieu M., LE FEVRE J. P. , Alis S., et al., "The XXL Survey II. The bright cluster sample: catalogue and luminosity function", ASTRONOMY & ASTROPHYSICS, cilt.592, 2016
dc.identifier.issn1432-0746
dc.identifier.othervv_1032021
dc.identifier.otherav_a0a876fe-4b4a-453c-9ec0-07fc07f239df
dc.identifier.urihttp://hdl.handle.net/20.500.12627/107730
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201526891
dc.description.abstractContext. The XXL Survey is the largest survey carried out by the XMM-Newton satellite and covers a total area of 50 square degrees distributed over two fields. It primarily aims at investigating the large-scale structures of the Universe using the distribution of galaxy clusters and active galactic nuclei as tracers of the matter distribution. The survey will ultimately uncover several hundreds of galaxy clusters out to a redshift of similar to 2 at a sensitivity of similar to 10 (14) erg s (1) cm (2) in the [0.5-2] keV band.
dc.language.isoeng
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectFizik
dc.titleThe XXL Survey II. The bright cluster sample: catalogue and luminosity function
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.department, ,
dc.identifier.volume592
dc.contributor.firstauthorID79486


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