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Probing reionization with LOFAR using 21-cm redshift space distortions

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dc.contributor.authorJensen, Hannes
dc.contributor.authorDatta, Kanan K.
dc.contributor.authorMellema, G.
dc.contributor.authorChapman, Emma
dc.contributor.authorAbdalla, Filipe B.
dc.contributor.authorIliev, I. T.
dc.contributor.authorMao, Yi
dc.contributor.authorSantos, Mario G.
dc.contributor.authorShapiro, Paul R.
dc.contributor.authorZaroubi, Saleem
dc.contributor.authorBernardi, G.
dc.contributor.authorBrentjens, Michiel A.
dc.contributor.authorde Bruyn, A. G.
dc.contributor.authorCiardi, Benedetta
dc.contributor.authorHarker, Geraint
dc.contributor.authorJelic, Vibor
dc.contributor.authorKazemi, S.
dc.contributor.authorKoopmans, L. V. E.
dc.contributor.authorLabropoulos, Panos
dc.contributor.authorMartinez, O.
dc.contributor.authorOffringa, Andre
dc.contributor.authorPandey, V. N.
dc.contributor.authorVeligatla, V.
dc.date.accessioned2015-12-13T22:30:45Z
dc.date.issued2013
dc.date.updated2016-02-24T09:25:03Z
dc.description.abstractOne of the most promising ways to study the epoch of reionization (EoR) is through radio observations of the redshifted 21-cm line emission from neutral hydrogen. These observations are complicated by the fact that the mapping of redshifts to line-of-sigh
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/74983
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Dark ages, reionization,first stars.; instrumentation: interferometers; Methods: numerical
dc.titleProbing reionization with LOFAR using 21-cm redshift space distortions
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage474
local.bibliographicCitation.startpage460
local.contributor.affiliationJensen, Hannes, Stockholm University
local.contributor.affiliationDatta, Kanan K., Stockholm University
local.contributor.affiliationMellema, G., Stockholm University
local.contributor.affiliationChapman, Emma, University College London
local.contributor.affiliationAbdalla, Filipe B, University College London
local.contributor.affiliationIliev, I. T., University of Sussex
local.contributor.affiliationMao, Yi, UPMC Univ Paris 06
local.contributor.affiliationSantos, Mario G., University of the Western Cape
local.contributor.affiliationShapiro, Paul R., University of Texas
local.contributor.affiliationZaroubi, Saleem, University of Groningen
local.contributor.affiliationBernardi, G, Harvard-Smithsonian Center for Astrophysics
local.contributor.affiliationBrentjens, Michiel A, ASTRON
local.contributor.affiliationde Bruyn, A G, University of Groningen Kapteyn Astronomical Institute
local.contributor.affiliationCiardi, Benedetta, Max-Planck-Institute for Astrophysics
local.contributor.affiliationHarker, Geraint, University of Colorado
local.contributor.affiliationJelic, VIBOR, ASTRON
local.contributor.affiliationKazemi, S., University of Groningen
local.contributor.affiliationKoopmans, L. V. E., Kapteyn Astronomical Institute
local.contributor.affiliationLabropoulos, Panos, ASTRON
local.contributor.affiliationMartinez, O., University of Groningen
local.contributor.affiliationOffringa, Andre, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationPandey, V N, ASTRON
local.contributor.affiliationVeligatla, V, University of Groningen
local.contributor.authoruidOffringa, Andre, u5259282
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB4409
local.identifier.citationvolume435
local.identifier.doi10.1093/mnras/stt1341
local.identifier.scopusID2-s2.0-84885098275
local.identifier.thomsonID000325804300031
local.type.statusPublished Version

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