dc.date.accessioned2020-03-11T20:36:12Z
dc.date.accessioned2022-10-18T23:02:56Z
dc.date.available2020-03-11T20:36:12Z
dc.date.available2022-10-18T23:02:56Z
dc.date.created2020-03-11T20:36:12Z
dc.date.issued2011
dc.identifierhttp://hdl.handle.net/10533/240890
dc.identifier15010003
dc.identifierWOS:000292392400005
dc.identifierno scielo
dc.identifiereid=2-s2.0-79961089146
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472229
dc.description.abstractWe report the first detection of the gravitational lensing of the cosmic microwave background through a measurement of the four-point correlation function in the temperature maps made by the Atacama Cosmology Telescope. We verify our detection by calculat
dc.languageeng
dc.relationhttps://doi.org/10.1103/PhysRevLett.107.021301
dc.relation10.1103/PhysRevLett.107.021301
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleDetection of the Power Spectrum of Cosmic Microwave Background Lensing by the Atacama Cosmology Telescope
dc.typeArticulo


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