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dc.contributor.authorUros Seljak-
dc.date.accessioned2016-08-28T10:08:51Z-
dc.date.available2016-08-28T10:08:51Z-
dc.date.issued2013-
dc.identifier.issn1475-7516-
dc.identifier.otherOAK-10696-
dc.identifier.urihttps://dspace.ewha.ac.kr/handle/2015.oak/224228-
dc.description.abstractcosmological perturbation theory; galaxy clustering; galaxy surveys; power spectrum-
dc.languageEnglish-
dc.titleDistribution function approach to redshift space distortions. Part V: Perturbation theory applied to dark matter halos-
dc.typeArticle-
dc.relation.issue10-
dc.relation.volume2013-
dc.relation.indexSCIE-
dc.relation.indexSCOPUS-
dc.relation.journaltitleJournal of Cosmology and Astroparticle Physics-
dc.identifier.doi10.1088/1475-7516/2013/10/053-
dc.identifier.wosidWOS:000326979500053-
dc.identifier.scopusid2-s2.0-84887655395-
dc.author.googleVlah Z.-
dc.author.googleSeljak U.-
dc.author.googleOkumura T.-
dc.author.googleDesjacques V.-
dc.contributor.scopusidUros Seljak(55508271200)-
dc.date.modifydate20230613102228-
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자연과학대학 > 물리학전공 > Journal papers
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