Joining bits and pieces of reionization history

dc.contributor.authorHazra, Dhiraj Kumar
dc.contributor.authorPaoletti, Daniela
dc.contributor.authorFinelli, Fabio
dc.contributor.authorSmoot, George F.
dc.date.accessioned2019-07-20T11:54:37Z
dc.date.available2019-07-20T11:54:37Z
dc.date.issued2019-04-02
dc.description.abstractCosmic Microwave Background temperature and polarization anisotropies from Planck have estimated lower value of the optical depth to reionization (τ) compared to WMAP.en_US
dc.identifier.citationHazra, D. K., Paoletti, D., Finelli, F., & Smoot, G. F. (2019). Joining bits and pieces of reionization history. Retrieved from http://arxiv.org/abs/1904.01547en_US
dc.identifier.other1904.01547
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/4046
dc.language.isoenen_US
dc.publisherNURIS; Energetic Cosmos Laboratoryen_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectThe 2nd international conference of the Energetic Cosmos Laboratory (ECL)en_US
dc.subjectECL19en_US
dc.subjectEnergetic Cosmos Laboratory (ECL)en_US
dc.titleJoining bits and pieces of reionization historyen_US
dc.typeArticleen_US
workflow.import.sourcescience

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