Jensen, HannesDatta, Kanan K.Mellema, G.Chapman, EmmaAbdalla, Filipe B.Iliev, I. T.Mao, YiSantos, Mario G.Shapiro, Paul R.Zaroubi, SaleemBernardi, G.Brentjens, Michiel A.de Bruyn, A. G.Ciardi, BenedettaHarker, GeraintJelic, ViborKazemi, S.Koopmans, L. V. E.Labropoulos, PanosMartinez, O.Offringa, AndrePandey, V. N.Veligatla, V.2015-12-130035-8711http://hdl.handle.net/1885/74983One 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-sighKeywords: Dark ages, reionization,first stars.; instrumentation: interferometers; Methods: numerical201310.1093/mnras/stt13412016-02-24