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dc.contributor.authorSERENO, M.
dc.contributor.authorMOSCARDINI, L.
dc.contributor.authorPACAUD, F.
dc.contributor.authorPierre, M.
dc.contributor.authorPLIONIS, M.
dc.contributor.authorCAPPI, A.
dc.contributor.authorADAMI, C.
dc.contributor.authorALTIERI, B.
dc.contributor.authorBirkinshaw, M.
dc.contributor.authorETTORI, S.
dc.contributor.authorFaccioli, L.
dc.contributor.authorGASTALDELLO, F.
dc.contributor.authorKoulouridis, E.
dc.contributor.authorLIDMAN, C.
dc.contributor.authorLE FEVRE, J. -P.
dc.contributor.authorMAUROGORDATO, S.
dc.contributor.authorPOGGIANTI, B.
dc.contributor.authorPOMPEI, E.
dc.contributor.authorSadibekova, T.
dc.contributor.authorVALTCHANOV, I.
dc.contributor.authorMARULLI, F.
dc.contributor.authorVEROPALUMBO, A.
dc.contributor.authorAlis, Sinan
dc.date.accessioned2021-03-05T16:02:28Z
dc.date.available2021-03-05T16:02:28Z
dc.identifier.citationMARULLI F., VEROPALUMBO A., SERENO M., MOSCARDINI L., PACAUD F., Pierre M., PLIONIS M., CAPPI A., ADAMI C., Alis S., et al., "The XXL Survey XVI. The clustering of X-ray selected galaxy clusters at z similar to 0.3", ASTRONOMY & ASTROPHYSICS, cilt.620, 2018
dc.identifier.issn1432-0746
dc.identifier.othervv_1032021
dc.identifier.otherav_bebe4133-3217-4f59-bec6-a8d688c3cfe8
dc.identifier.urihttp://hdl.handle.net/20.500.12627/126665
dc.identifier.urihttps://doi.org/10.1051/0004-6361/201833238
dc.description.abstractContext. Galaxy clusters trace the highest density peaks in the large-scale structure of the Universe. Their clustering provides a powerful probe that can be exploited in combination with cluster mass measurements to strengthen the cosmological constraints provided by cluster number counts.
dc.language.isoeng
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleThe XXL Survey XVI. The clustering of X-ray selected galaxy clusters at z similar to 0.3
dc.typeMakale
dc.relation.journalASTRONOMY & ASTROPHYSICS
dc.contributor.department, ,
dc.identifier.volume620
dc.contributor.firstauthorID79600


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