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Using the full power of the cosmic microwave background to probe axion dark matter

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dc.bibliographiccitation.firstpage3063
dc.bibliographiccitation.issue3
dc.bibliographiccitation.journalMonthly Notices of the Royal Astronomical Society
dc.bibliographiccitation.lastpage3085
dc.bibliographiccitation.volume476
dc.contributor.authorHložek, Renée
dc.contributor.authorMarsh, David J E
dc.contributor.authorGrin, Daniel
dc.date.accessioned2020-12-10T18:19:30Z
dc.date.available2020-12-10T18:19:30Z
dc.date.issued2018
dc.identifier.doi10.1093/mnras/sty271
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://resolver.sub.uni-goettingen.de/purl?gro-2/75268
dc.language.isoen
dc.notes.internDOI Import GROB-354
dc.titleUsing the full power of the cosmic microwave background to probe axion dark matter
dc.typejournal_article
dc.type.internalPublicationyes
dspace.entity.typePublication

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