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pro vyhledávání: '"X rays, Cosmological parameters"'
The possibility of determining the value of the Hubble constant using observations of galaxy clusters in X-ray and microwave wavelengths through the Sunyaev Zeldovich (SZ) effect has long been known. Previous measurements have been plagued by relativ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::91401a031b73998d0df3ad4fb0747cb5
http://hdl.handle.net/20.500.12386/29562
http://hdl.handle.net/20.500.12386/29562
