The hyperfine transition of 3He+ as a probe of the intergalactic medium

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We explore the prospects of using the hyperfine transition of 3He+ as a probe of the intergalactic medium. The emission signal from ionized regions during reionization is expected to be anti-correlated with 21cm maps. The predicted emission signal from Lyman-alpha blobs at lower redshifts is detectable with future radio observatories.
5 pages, 1 figure, submitted to MNRAS

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